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CHARGE CARRIER RECOMBINATION IN AMORPHOUS SELENIUM FILMS A Thesis Submitted to the College of Graduate Studies and Research in Partial Fulfillment of the Requirements for the Degree of Master of Science in the Department of Electrical Engineering University of Saskatchewan Saskatoon by CHRISTOPHER JON HAUGEN Saskatoon, Saskatchewan May 1995 Copyright © 1994: Christopher Jon Haugen

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Page 1: CHARGE CARRIER RECOMBINATION IN AMORPHOUS SELENIUM …

CHARGE CARRIER RECOMBINATION

IN AMORPHOUS SELENIUM FILMS

A Thesis

Submitted to the College of Graduate Studies and Research

in Partial Fulfillment of the Requirements

for the Degree of

Master of Science

in the Department of Electrical Engineering

University of Saskatchewan

Saskatoon

by

CHRISTOPHER JON HAUGEN

Saskatoon, Saskatchewan

May 1995

Copyright © 1994: Christopher Jon Haugen

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COPYRIGHT

The author has agreed that the Library, University of Saskatchewan,

may make this thesis freely available for inspection. Moreover, the author

has agreed that permission for extensive copying of this thesis for scholarly

purposes may be granted by the professor who supervised the thesis work

recorded herein, or in his absence, by the Head of the Department or the

Dean of the College in which this thesis work was done. It is understood

that due recognition will be given to the author of this thesis and to the

University of Saskatchewan in any use of the material in this thesis.

Copying or publication or any other use of this thesis for financial gain

without approval by the University of Saskatchewan and the author's

written permission is prohibited.

Requests for permission to copy or make any other use of the material

in this thesis in whole or in part should be addressed to:

Head of Department of Electrical Engineering

University of Saskatchewan

Saskatoon, Canada, S7N OWO

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University of Saskatchewan

Electrical Engineering Abstract # 94A408

CHARGE CARRIER RECOMBINATION IN AMORPHOUS SELENIUM FILMS

Student: C. Haugen Supervisor: Dr. S.O. Kasap

M. Sc. Thesis Submitted to the College of Graduate Studies and Research

August 1994

ABSTRACT

The charge transport characteristics of amorphous semiconductors determine how well they will perform in many applications. The product of the charge carrier drift mobility, µ, and deep trapping lifetime, t, also known as the range of the carrier, represents the average distance per unit electric field that a charge carrier will travel in the conduction band before being trapped in deep localized states within the mobility gap. The irc product is therefore an important parameter in predicting the performance of an amorphous semiconductor based device. However, in applications where more than one polarity of electronic charge is involved, charge carrier recombination is also an important consideration. The use of amorphous selenium alloy based films in electroradiography is one such application. This work utilized three different experimental techniques to determine charge carrier drift mobility, deep trapping lifetime and recombination coefficient in stabilized amorphous selenium (a-Se:0.2%As+Cl in ppm) films, suitable for use in electroradiographic systems. The conventional time-of-flight (TOF) method was used to evaluate carrier drift mobility and the interrupted field time-of-flight (IFTOF) technique was used to determine the carrier deep trapping lifetime. The hole range of the amorphous selenium films used was wth=67.54x10-6 cm2V-1, and the electron range was wre=2.68x10-6 cm2V-1. An ambipolar time-of-flight experiment was performed to measure bulk recombination by measuring the fractional change in hole photocurrent as an electron and hole charge packet passed through each other under the influence of an applied field.

TOF and IFTOF measurements were used to characterize charge transport in the samples before the recombination experiment was performed. The ambipolar TOF experiment indicated that the charge carrier recombination process within chlorinated a-Se:0.2%As follows the

ii

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Langevin process, originally proposed for recombination of gaseous ions. The predicted Langevin recombination coefficient was Cer=35.2x10-9 cm3s-1, while the experimentally determined Langevin recombination coefficient was CrE=36.6x10-9 cm3s-1. This implies that the carrier mean free path in the films is much less than the recombination radius defined by Langevin. As most photoinduced discharge theories ignore the effect of carrier recombination their development, the measured recombination coefficient can now be used to reformulate these models to include recombination.

in

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ACKNOWLEDGMENTS

I would like to extend my sincere thanks to my supervisor, Professor

S.O. Kasap, for his guidance, help and friendship during the course of this

project. My thanks are extended to Brad Polischuk (at Noranda Technology

Centre) for providing the IFTOF measurements and for the many insightful

discussions. I am grateful to Noranda Technology Centre for providing the

sample materials and for supplementary financial help. I would also like to

express my appreciation to NSERC for the financial support I have received.

Finally, I would like to thank my wife Laura for her unfailing support,

encouragement, and patience.

iv

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TABLE OF CONTENTS

COPYRIGHT

ABSTRACT ii

ACKNOWLEGDEMENTS iv

TABLE OF CONTENTS

LIST OF FIGURES vii

LIST OF ABBREVIATIONS xi

1. INTRODUCTION 1 1.1 Introduction 1 1.2 Applications of Amorphous Selenium 2

1.2.1 Electrophotographic Photoreceptors 2 1.2.2 Electroradiographic Detectors 5

1.3 Research Objectives 8 1.4 Thesis Outline 9

2. PROPERTIES OF AMORPHOUS SELENIUM 10 2.1 Introduction 10 2.2 Structure of Amorphous Selenium 10 2.3 Band Model for Amorphous Selenium 13 2.4 Optical Properties of Amorphous Selenium 16 2.5 Charge Transport in Amorphous Selenium 19 2.6 Summary 24

3. TIME-OF-FLIGHT AND AMBIPOLAR RECOMBINATION EXPERIMENTS 26 3.1 Introduction 26 3.2 Principles of the Time-of-Flight (TOF) Technique 27 3.3 Transient Trap Limited Theory 35

3.3.1 tc«tx<tT Case 39 3.3.2 High Field Case (tT<Tc) 40

3.4 Summary 41

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4. EXPERIMENTAL PROCEDURE 43 4.1 Introduction 43 4.2 Sample Preparation 43 4.3 Ambipolar Time-Of-Flight (TOF) Apparatus 47

4.3.1 Photoexcitation Sources 50 4.3.1.1 Xenon Flash Bulb Source 50 4.3.1.2 Nitrogen Laser Source 53

4.3.2 Timing Signal Generator 56 4.3.3 Digital Delays 59 4.3.4 Bias Application Circuit 59 4.3.5 Voltage Follower Circuit 60 4.3.6 Data Acquisition System 61

4.4 Interrupted Field Time-of-Flight (IFTOF) Apparatus 63 4.4.1 Schering Bridge Network 69 4.4.2 High Voltage TMOS Switch 71

4.5 Summary 72

5. RESULTS AND DISCUSSION 73 5.1 Introduction 73 5.2 Charge Transport Study 73 5.3 Charge Trapping Study 78 5.4 Ambipolar Recombination Experiment 82 5.5 Summary 91

6. CONCLUSIONS 93

7. REFERENCES 97

vi

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LIST OF FIGURES

Figure 1.1 The basic steps of the xerographic process: (1)charge, (2) expose, (3) develop, (4) transfer, (5) fix, (6) clean, and (7) erase. 3

Figure 1.2 Typical projection radiographic system for medical imaging 5

Figure 1.3 Development system for electroradiography consisting of a pulsed laser beam and capacitively coupled probe. 7

Figure 2.1 Atomic arrangements in (a) a perfect crystal and (b) a perfect network glass 11

Figure 2.2 Selenium chain molecule and the definition of the dihedral angle 4). The dihedral angle is formed by the planes defined by atoms 123 and 234 12

Figure 2.3 Local structure of amorphous selenium showing chainlike segments of y-Se and ringlike segments of a-Se. 13

Figure 2.4 Various forms proposed for the density of states as a function of energy for crystalline and amorphous semiconductors. (a) crystalline model (b) Mott's model, (c) CFO model, and (d) Davis-Mott model [11]. 15

Figure 2.5 Experimentally determined density of states function N(E) for a-Se [12]. 16

Figure 2.6 Absorption coefficient a and quantum efficiency Tl as a function of the incident photon energy hv for various applied fields F [13,15]. 18

Figure 2.7 Predicted variation of carrier mobility in amorphous solids with energy [16]. 20

vii

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Figure 2.8 Energy diagram for an electron bound to a point charge in the presence of a uniform electric field (Poole-Frenkel effect) [21]. 23

Figure 3.1 (a) Simplified schematic and (b) small signal ac equivalent circuit for the Time-of-Flight transient photoconductivity technique, where Cs is the sample capacitance. 28

Figure 3.2 The motion of charge q through dx induces charge dQ to flow through the external circuit. 30

Figure 3.3 Signals from the TOF experiment where (a) and (b) are I-mode signals for the trap free and deep trapping only case and (c) and (d) are V-mode signals for the same cases [20]. 34

Figure 3.4 Current flow with trapping and release processes in a thin slice of thickness dx. 36

Figure 4.1 Schematic diagram of the vacuum deposition system 45

Figure 4.2 Schematic diagram of sputtering system 46

Figure 4.3 Generalized schematic of TOF experiment 48

Figure 4.4 Diagrammatic view of ambipolar TOF experiment apparatus. 50

Figure 4.5 Schematic sketch of xenon flash circuit. 52

Figure 4.6 a)Reverse biased p-i-n measurement circuit. b)Light output Vs time for xenon flash. Horizontal axis: 200ns/div.; Vertical axis: 20mV/div. 53

Figure 4.7 Potential energy curves for lowest triplet states in N2 molecule 54

Figure 4.8 Blumlein circuit used for rapid excitation of N2

laser. 55

Figure 4.9 Triggering requirements for the LN 103 C N2 laser. 56

viii

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Figure 4.10

Figure 4.11

Figure 4.12

Figure 4.13

Figure 4.14

Figure 4.15

Figure 4.16

Figure 4.17

Figure 4.18

Figure 4.19

Figure 5.1

Timing signals from Timing Signal Generator. twD, iTi, AT2, and An are adjustable as shown in Figure 4.11. 57

Circuit diagram for TTL trigger signal generator. 58

Schematic of pulsed bias application circuit. 60

Schematic of voltage follower with protection relay. 61

Diagrammatic layout of data acquisition system. The system features include the C1002 CCD camera, Tektronix 2467B oscilloscope, an IBM compatible PC to house the frame storage board and run the DCS01 software, and the Panasonic VW-5350 video monitor. 62

(a)Timing sequence for the application of bias voltage in TOF experiment and (b) the resulting photocurrent waveform. (c)The timing signal for the application of the bias in the IFTOF experiment and (d) the resulting IFTOF photocurrent signal 65

Large displacement current signals are produced when the high voltage bias is switched on and off. This signal must be eliminated for the IFTOF experiment to be successfully implemented. 67

IFTOF experiment schematic based on the Schering bridge network. 68

Schematic of Schering bridge network used to implement displacement current signal free IFTOF measurements. 69

Schematic of TMOS high voltage switch. 71

Conventional I-mode TOF waveforms for a 195.1 gm a-Se:0.2%As film for (a) hole transit and (b) electron transit. The transit times are indicated by tT 75

ix

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Figure 5.2

Figure 5.3

Figure 5.4

Figure 5.5

Figure 5.6

Figure 5.7

Figure 5.8

Figure 5.9

Figure 5.10

Figure 5.11

TOF plot of transit time versus 1/voltage for holes in a-Se:0.2%As film showing µh =0.125 cm2V-ls-1 76

TOF plot of transit time versus 1/voltage for electrons in a-Se:0.2%As film shoWing 1.4=0.0034 cm2V-Is-1 76

Plot of hole and electron mobility as a function of the applied electric field. The hole mobility shows no observable field dependence. The electron mobility shows a very slight field dependence of the form g em F0.04 77

Typical IFTOF waveform for holes in a 195.1 p.m a-Se:0.2%As film showing i(ti), i(t2), and t1. 80

Logarithm of fractional recovered photocurrent as a function of interruption time for holes in a-Se:0.2%As. 81

Logarithm of fractional recovered photocurrent as a function of interruption time for electrons in a-Se:0.2%As. 81

(a) Simplified schematic sketch of double injection TOF technique for studying recombination and (b) the resulting photocurrent. 85

A typical photocurrent waveform from ambipolar TOF experiment. Insert shows an expanded view of the photocurrent due to the hole packet "riding" the top of the electron packet signal. 86

Schematic diagram of hole and electron packets passing through each other. It is assumed that n(x,t)»p(x,t). 87

Semilogarithmic plot for ihilim versus ae/F for two different stabilized a-Se samples. The slope of the line gives a relative dielectric constant of er=6.35. Correlation coefficient r=0.94.. 91

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LIST OF ABBREVIATIONS

a-Se amorphous selenium

a-Si:H hydrogenated amorphous selenium

CCD charge coupled device

CFO density of states model proposed by Cohen, Fritzsche, and Ovshinski.

CuSO4 copper sulphate

DDG digital delay generator

EHP electron-hole pair

ESR electron spin resonance

IFTOF interrupted field time-of-flight

PVC polyvinyl-chloride

PVK:TNF poly-n-vinylcarbazole:trinitrofluorenone

TEA transversely excited atmospheric

TP transient photoconductivity

VAP valence alteration pair.

xi

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1 INTRODUCTION

1.1 Introduction

Quantum mechanical theory was developed in the 1920s and 1930s.

The theory of quantum mechanics was readily applied to the study of the

physical behaviour of crystalline solids due to the mathematical simplicities

that resulted when dealing with a periodic structure. This led to the

development of many crystalline-based devices, the most important of which

was the solid state transistor.

However, due to the complexities of applying quantum mechanical

models to non-periodic structures, device physics based on amorphous solids

did not experience the same rapid growth as for crystalline materials. Much

of the theoretical understanding of the properties of non-crystalline

materials has been derived since the 1960s. Despite this, it is quite possible

that amorphous semiconductors will become the basis for the next era of

growth in the microelectronics industry [1]. In general terms, amorphous

materials possess a far greater diversity in their physical properties than do

crystalline materials. Furthermore, the preparation of amorphous solids

does not usually require the same carefully controlled growth techniques.

This provides a tremendous economical advantage for many applications.

1

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1.2 Applications of Amorphous Selenium

One group of commercially important amorphous materials are the

chalcogenide glasses and in particular amorphous selenium and its alloys.

Since the first paper published on the photoconductive properties of

selenium in 1873 [2], selenium has gone on to be used in a large variety of

applications including providing sound for early motion pictures,

xerography, electroradiographic detection, and use in TV pickup tubes. Of

these applications, xerography and electroradiography are the most

important for this work.

1.2.1 Electrophotographic Photoreceptors

The electrophotographic, or xerographic, industry started in 1938

with the invention of the electrophotographic copier by Chester Carlson [3].

The industry has since grown into a 100 billion dollar/year commercial

enterprise. Today, it encompasses many different forms of

electrophotography including copying machines, fax machines, scanners,

and laser printers. Amorphous selenium photoreceptors were the first to be

used commercially in the early 1960s and continue to be widely used, though

their importance has recently shifted to electroradiography.

The seven basic steps in the xerographic process are shown in Figure

1.1. The first step is to charge the photoconductor. The most common

method used for the charging process is corona discharge. A high electric

field is applied to a thin wire (corotron) which in turn generates a plasma

around itself. Ions drift from the plasma to the surface of the

2

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photoconductor thereby charging it uniformly. Next, the photoreceptor is

light-exposed to the optical image to be reproduced.

(1) Charge

Document Toner Particles

44) RFA) gar) .

(2) Expose

(4) Transfer

Photoreceptor

1 Twee. 1

Photoreceptor 4 (3) Develop

wpIem. !die..

Paper

(5) Fix

6 Lamp

1

Photoreceptor

(6) Clean (7) Erase

Fuser Roller 150-200 e Pressure Roller 40-80

Figure 1.1 The basic steps of the xerographic process: (1)charge, (2) expose, (3) develop, (4) transfer, (5) fix, (6) clean, and (7) erase.

3

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The light areas of the image cause the corresponding area on the

photoreceptor to discharge through a photoconductive process, while the

corresponding dark areas remain charged. This creates a latent electrostatic

image on the surface of the photoreceptor. The latent image is then

developed by using electrostatically charged toner particles. The particles

stick to the oppositely charged latent image. The particles are then

transferred to the paper, by positively charging the back of the sheet, and

fused by heating the particles to form the final hard copy. Before another

image can be made, the remaining toner particles must be cleaned from the

photoreceptor and any residual electrostatic charge from the image is erased

by flooding the photoreceptor with a uniform high intensity light.

- The amount of photoconductive discharge that occurs during the

formation of the latent image is determined by the electronic properties of

the photoreceptor. The average distance per unit electric field that a charge

carrier will move in the photoconductor is termed the range of the carrier.

The range is given by the i.rt product where µ is the drift mobility, and ti is

the deep trapping lifetime of the carrier. Consequently, the product of the

applied field and the carrier range will determine the average distance

traveled by the charge. For optimal photodischarge, the photogenerated

carriers must move distances greater than the thickness of the

photoconductive layer. Therefore, the charge carrier drift mobility and deep

trapping lifetime are very important parameters for characterizing the

performance of the photoreceptor.

4

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1.2.2 Electroradiographic Detectors

The use of amorphous selenium in x-ray imaging has been well

documented and continues to be a field of intensive research [4,5]. There is

considerable interest in digital electroradiogaphy where an electrostatic

image on an x-ray plate is read and converted to a digital form for computer

storage and processing [6].

The medical imaging application of electroradiography relies on the

differential absorption of ionizing radiation by different tissues in the

human body. A typical projection radiographic systems consists in its most

general form of an x-ray source and an x-ray sensitive detector which is

placed behind the subject as shown in Figure 1.2.

X-ray Detector

X-ray Source

Figure 1.2 Typical projection radiographic system for medical imaging.

5

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The patient is exposed to the x-rays and the differential attenuation of

the x-rays in passing through the body modulates the radiation intensity

that reaches the detector. The detector must then store this information

until a visible image can be made. Conventional detectors consist of a

photographic film cassette which is sandwiched between fluorescent screens.

Incident radiation which strikes the screens is converted into light which is

then recorded by the film. The film is then developed using standard

photographic means to view the image.

In electroradiography, the photographic cassette is replaced with a

solid-state, planar, image detector. The detector is charged, similar to the

xerographic process, and when exposed to the x-ray radiation undergoes

photodischarge. This leaves a latent electrostatic image on the surface of

the detector. This image may be read by using the sequential discharge of

the surface by a scanning pulsed laser beam and capacitively coupled

transparent probe system shown in Figure 1.3 [6]. The sampling electrode is

capacitively coupled to the surface of the detector. The electrode assumes a

potential related to the surface charge on the detector and the degree

of coupling. When the laser is focused onto the detector, the charge on the

surface of the detector undergoes photodischarge. The sensing electrode

records a change in charge proportional to the change in surface charge.

The image is reconstructed by correlating the electrode voltage signal with

the path of the laser beam. The image can then be stored and analyzed by a

computer.

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Transparent Electrode

Conducting Layer

Pulsed Scanning Laser Beam

+ + ++ ++ a-Se Film

Al Substrate

0

Figure 1.3 Development system for electroradiography consisting of a pulsed laser beam and capacitively coupled probe.

There are three major advantages to the electroradiographic system

over the conventional system. First, by replacing the photographic film, the

process is changed from a chemical to an electronic process. This has

environmental as well as economic implications in that the imaging plates

are fully reusable and the costs of the chemical purchase and reclamation

are removed.

Secondly, research on selenium based x-ray detectors indicates that

they are more sensitive to x-ray radiation than conventional film detectors.

This means that for comparable image quality, the patient is exposed to

lower radiation levels when using the solid state detector. This increases

the safety factor for the patient.

Finally, solid state detectors allow for a higher lateral resolution than

photographic detectors. Light that is generated in fluorescent screens of the

photographic cassettes propagate to the surface of the film through an

isotropic diffusion process, i.e. they spread parallel as well as perpendicular

to the image plane. This limits the resolution on the film. This problem is

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overcome in the solid state detector since the charge carriers involved with

electrostatic discharge move along the applied electric field and therefore

perpendicular to the image plane.

Since the imaging process is based on photoinduced discharge, the

range or wr product is a very important material parameter for studying the

detectors used in electroradiography. However, carriers in selenium

electroradiographic detectors are not lost to conduction through deep

trapping alone. Charge carrier recombination may also play an important

role. The x-ray absorption process for amorphous selenium is such that

electron-hole pairs are generated throughout the bulk of the detector. The

application of an electric field causes the electrons and holes to move past

each other, and there is a probability that some carriers recombine. The

recombination coefficient, Cr, is therefore another important parameter for

characterizing the usefulness of a material as a detector.

1.3 Research Objectives

Amorphous semiconductors have been the subject of a great deal of

scientific interest and study. As their use increases, it becomes more

important to understand the physical and electronic properties of this group

of materials. The primary focus of this research is to study charge carrier

recombination in chlorinated a-Se:0.2%As films suitable for use in

electroradiographic systems.

The experimental techniques used were the time-of-flight (TOF)

technique, the interrupted field time-of-flight (IFTOF) technique, and a

8

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double flash, ambipolar time-of-flight technique. The results from the TOF

and IFTOF experiments were used to characterize charge transport, i.e. wr

product, in the films. The ambipolar TOF technique was used to directly

measure the amount of recombination that occurred within the samples

when holes and electrons interacted with one another.

1.4 Thesis Outline

This thesis is divided into six chapters. Following this introductory

chapter, a brief review of the various structural, optical, and electronic

properties of amorphous selenium is given in Chapter 2. Chapter 3 provides

the principle of the time-of flight transient photoconductivity technique and

an analytical framework for studying charge transport in a material with a

single species of traps. A description of the ambipolar TOF and IFTOF

measurement systems used in this work is provided in Chapter 4 along with

a description of the sample preparation procedure. Chapter 5 presents the

results from the TOF, IFTOF and ambipolar recombination measurements

performed on amorphous selenium films. Finally, the conclusions drawn

from the results in Chapter 5 are presented in Chapter 6, along with some

recommendations for future work.

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2. PROPERTIES OF AMORPHOUS SELENIUM

2.1 Introduction

This chapter deals with the physical properties of amorphous

selenium. The physical structure of amorphous selenium and its energy

band model are described. These determine the optical and electrical

properties the material exhibits. .

2.2 Structure of Amorphous Selenium

Amorphous and crystalline materials have vastly different structures.

Figure 2.1 presents in schematic fashion the atomic arrangement of a

perfectly crystalline material as opposed to a perfect network glass. The

dots in the figure represent the equilibrium positions about which the atoms

oscillate. In a perfect crystal, the bonding arrangement (i.e. bond length and

bond angle) for each atom is identical regardless of the atom's position in the

crystal. The crystalline solid exhibits a translational periodicity and

possesses "long range order". This does not hold for amorphous solids.

Atoms in an amorphous solid have slight variations in bond length and bond

angle which destroy the periodicity for distances greater than a few atomic

radii. The amorphous solid does however exhibit a high degree of short

range order. The valency requirements for each atom in the structure are

10

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satisfied and each atom is normally bonded to the same number of

neighbouring atoms.

(a) (b)

Figure 2.1 Atomic arrangements in (a) a perfect crystal and (b) a perfect network glass.

In the crystalline state, selenium can exist in one of two forms,

monoclinic Se (a - Se) and trigonal Se (y-Se). a-Se is composed of Ses rings

while y-Se comprises of parallel Se. spiral chains in a hexagonal structure.

It is natural to assume that the structure of amorphous selenium • would

preserve elements of a-Se and y-Se, that is a mixture of ring and chain

members. Recent studies on the structure of amorphous selenium now

favour a "random chain model" with all the atoms in a twofold coordinated

chain structure. The dihedral angle 4) of this chain remains constant in

magnitude but changes sign randomly [7].

Consider Figure 2.2 with atoms 1, 2, 3 and 4. The dihedral angle 4) is

defined as the angle between two adjacent bonding planes. It is observed in

Figure 2.2 by looking down the bond that connects atoms 2 and 3. In y-Se,

11

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the dihedral angle rotates in the same sense in moving along the chain to

give a spiral pitch of three atoms. In a-Se, the dihedral angle alternates its

sign to form a ringlike structure. In the amorphous structure, the sign of

the dihedral angle changes randomly leading to regions that are chain-like

and to regions that are ring-like as in Figure 2.3.

Figure 2.2 Selenium chain molecule and the definition of the dihedral angle (1). The dihedral angle is formed by the planes defined by atoms 123 and 234.

Although the twofold coordinated structure, Se2°, is the most

energetically favourable, thermally derived charged structural defects,

known as Valence Alternation Pairs (VAPs), also exist in the amorphous

state. These VAPs correspond to some of the Se atoms being over- and

under-coordinated [8]. Electron Spin Resonance (ESR) studies have shown

that the lowest energy defects in amorphous selenium (a-Se) do not have

dangling bonds. It has also been calculated that the lowest energy defects

are not singly bonded Sei° or triply bonded Se3° atoms [52]. The lowest

energy defects are charged centres with paired electron spins, Sec and See.

12

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These structured defect pairs are the VAP, and they constitute the origin of

localized states within the mobility gap of the material.

Figure 2.3 Local structure of amorphous selenium showing chainlike segments of y-Se and ringlike segments of a-Se.

2.3 Band Model for Amorphous Selenium

The disorder inherent with amorphous materials results in a different

band structure from that of crystalline solids. A number of band models

have been proposed for amorphous materials.

Mott [9] took the first step in generalizing the quantum mechanical

arguments made for the band structure of crystalline semiconductors to

amorphous ones. Mott realized that quantum mechanical solutions for

crystals, that led to a density of states model where electrons existed in

13

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bands of extended states separated by gaps with sharp band edges, as in

Figure 2.4(a), were the result of the long range order in the crystal. He

argued that the lack of long range order in amorphous materials would

cause the sharp edged bands in crystalline materials to be replaced by bands

with tails of localized states. Mott further argued that extended states

would exist in amorphous materials at some particular density of electronic

states. This would in turn lead to a sharp increase in mobility at the critical

energy where the extended states began. This concept of a "mobility gap" in

amorphous solids is similar to the band gap concept for crystalline solids.

The density of states model proposed by Mott is shown in Figure 2.4(b).

Mott's original model was further expanded by Cohen, Fritzche, and

Ovshinsky [10]. Their model became known as the CFO Model and is shown

in Figure 2.4(c). This model assumed that the nature of the localized band

tails depends on the extent that the amorphous structures deviated from a

perfect periodicity. They postulated that the degree of disorder in

amorphous solids was greater than that assumed by Mott. As a result, the

band tails would extend through the mobility gap and give rise to a finite

density of states at the Fermi level (i.e. they would overlap). However, this

continuum of states in the gap would not give rise to metallic conduction

properties because the states were still assumed to be highly localized in

space. Finally, the CFO model considered that since amorphous material do

not have the rigid constraints of a crystalline material, each atom would

ordinarily be able to locally fulfill its valency requirements. This would

eliminate any sharp structure in the density of localized states in the

mobility gap.

14

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Ec

EF

E v

(a)

(c)

N(E)

N(E)

(b) N(E)

(d) N(E)

Figure 2.4 Various forms proposed for the density of states as a function of energy for crystalline and amorphous semiconductors. (a) crystalline model (b) Mott's model, (c) CFO model, and (d) Davis-Mott model [11].

However, amorphous semiconductors are thought to contain defects

such as impurities and dangling bonds. These may lead to discrete levels in

the mobility gap. This led Davis and Mott to relax the valency condition of

the CFO Model to account for the effects of structural defect [11]. The

Davis-Mott Model is shown in Figure 2.4(d).

15

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The currently accepted electronic density of states model, for a-Se is

shown in Figure 2.5 [12]. It was developed from various xerographic and

transient photoconductivity measurements. The high concentration of

shallow traps at energies -0.29eV above Ev and -0.35eV below Ec control

hole and electron drift mobilities through a shallow-trap-controlled band

transport process.

Ec

2.0 -

Ev 0

EF= 1.06 eV ••• *ft

og.

2.22 eV

I.-. I

1011 12 13 14 15 16

101710 10 10 10 10 1018

1019

1020

1021

N(E), cni3eV

Figure 2.5 Experimentally determined density of states function N(E) for a-Se [12].

2.4 Optical Properties of Amorphous Selenium

The task of a photoreceptor is to convert the photons of an incident

light signal into mobile charge carriers. Therefore, the optical properties of

16

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a material determine its value as a photoreceptive material. In an ideal

photoreceptor, each incident photon leads to the generation of an electron-

hole pair. Real materials however do not conform to this ideal behaviour.

The first optical property of importance to look at is the optical

absorption coefficient a. Optical absorption in semiconductors is determined

by the probability that a photon will excite an electron across the bandgap

and generate an electron-hole pair (EHP). As such, a depends on the photon

energy and the density of states at the band edges. As long as the photon

energy is less than the gap energy, little or no absorption will occur.

Studies reveal that the optical absorption coefficient of amorphous

selenium exhibits an Urbach edge of the form a=7.35x10-12

exp[hv/0.0058eV]cm-1 [13]. However, at high photon energies, the

absorption coefficient has been found to obey (ahv)-(hv-Eo) [14], where

E0-2.05eV is the optical bandgap at room temperature.

The second important optical property to be looked at is the quantum

efficiency of the photoreceptor. Quantum efficiency determines the

probability that generated EHPs will dissociate to form free electrons and

holes. For crystalline semiconductors, the quantum efficiency is largely

determined by recombination kinetics and is generally independent of

electric field and temperature. This is not the case with amorphous

selenium and many other low mobility solids.

The quantum efficiency of a-Se has a strong electric field dependence

even for photon energies greater than the mobility gap. Figure 2.6 shows

17

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the dependence of the absorption coefficient a and the quantum efficiency

on the photon energy hv.

E U

Abs

orpt

ion

Coe

ffic

ient

105

104

103

102

10

1

1

10-1

-2 10

103

104

10-5

101 10-6 1.5 2.0 2.5 3.0 3.5 4.0

Photon Energy hv, (eV) Q

uant

um E

ffic

ienc

y,

Figure 2.6 Absorption coefficient a and quantum efficiency ri as a function of the incident photon energy hv for various applied fields F [13,15].

The mechanism for the field dependent quantum efficiency in

amorphous selenium has been explained by the Onsager theory[15]. The

Onsager theory calculates the probability that an EHP will dissociate, as a

result of diffusion, under an electric field. The quantum efficiency depends

on the electric field F, the temperature T, and the initial separation of the

EHP ro. Thus, the quantum efficiency is given by

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11=110f(F,T,ro), (2.1)

where f(F,T,ro) is the probability that the EHP will dissociate and lio(hv) is

the quantum efficiency of the intrinsic photogeneration process.

2.5 Charge Transport in Amorphous Selenium

Assuming the existence of disorder-induced localized states within the

mobility gap, a number of charge transport mechanisms exist for amorphous

solids. As shown in Figure 2.7, electrons with energy far in excess of Ec

move in the extended electronic states. Conduction in these states is similar

to that of electrons in the conduction band of crystalline semiconductors. The

mean free path of the electron in these states is much longer than the

average interatomic distance and transport is based on Bloch wave

functions. The predicted mobility for carriers in these states is in excess of

100 cm2V-1s-1.

In the extended states just above the mobility edge, the long range

disorder of the material starts to dominate the transport process. The

carrier mean free path is comparable to the interatomic distance in these

states and charge transport can no longer be regarded as simple band

transport. Electron motion in these states is described as diffusive motion,

similar to Brownian motion [17]. The mobility in these states is of the order

of 1 cm2V-1s-1.

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CM2V -1S.1

µ>100

1 • • • • • * • •

• •-•-..* 11. < 10 -2

• • • •

11« 10 -2• • •

Figure 2.7 Predicted variation of carrier mobility in amorphous solids with energy [16].

Bloch wave functions do not extend throughout the material in the

localized states below Ec, but decay as exp(-aR) where R is the average

interatomic distance and a defines the rate at which the Bloch wave

function decays. The possibility exists that transport between these

localized states will occur by tunneling between the states. This 'hopping'

transport will depend on the overlap of wavefunctions between nearest

neighbours given by exp(-2aR), an attempt to hop frequency (i.e. phonon

frequency), VPH, and any activation energy, W, associated with the hopping

mechanism. Spear has described the mobility for such 'hopping' transport as

[18],

20

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eR 2 wl exp[-20cR]expt—Tri

kT (2.2)

The mobility for the hopping mechanism is estimated to be of the order of

10-2 cm2V-1s-1.

The exact nature of the microscopic mobility has not been conclusively

determined for amorphous selenium. Drift mobility studies have shown that

the thermally activated mobility has no pressure dependence [19]. This has

been used as evidence against a hopping transport mechanism and a

diffusive type transport in the extended states near the mobility edge has

been assumed.

In a material such as a-Se, which has a significant number of

localized states, the microscopic mobility go can be modulated by traps that

lie at lower energy levels with respect to the microscopic conduction level.

The drift of the carriers is periodically interrupted by capture and release

events from these shallow traps. The time spent by the carriers in the traps

effectively lowers the microscopic drift mobility of the carriers. go for such

carriers is reduced by a factor tc/(tc+TR) to µa where tc is the amount of time

the carrier remains free and Tx is the amount of time the carrier remains in

the trap. This conduction mechanism is known as trap-controlled transport

and has been observed in a-Se by examining the drift mobility at low

temperatures [20,50].

Carriers can be captured by three different types of traps: (a) centres

with an opposite electronic charge from the carrier (Coulomb attractive); (b)

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neutral centres; or (c) centres with the same electronic charge as the carrier

(Coulomb repulsive) [21]. Regardless of the type of trap involved, the

probability that a carrier will become captured is given by

1 _ NTCT, ,LC (2.3)

where tic is the mean free time before the carrier is captured, NT is the

density of traps and CT is the capture coefficient which is dependent on the

species of trap involved.

Charge carriers can be re-emitted from traps by a variety of different

mechanisms. Re-emission from a Coulomb-attractive trap is a thermally

activated process. The probability per unit time for thermal release from

this type of trap is given by Boltzmann statistics as

1 E T 1 = V exp[--

kT R (2.4)

where TR is the mean release time, vpH is an attempt to escape frequency

(phonon frequency), and ET is the depth of the trap below the band edge.

Further, it should be noted that if trap-controlled transport is applicable,

detailed balance considerations relate the trapping and de-trapping times by

a. N pPE ] TR NT

ex kT

22

(2.5)

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where Nc is the density of states in the conduction band.

The application of an electric field enhances re-emission from the

trapping centres. The applied field reduces the potential barrier in a

Coulomb-attractive trap through the Poole-Frenkel effect. This is illustrated

in Figure 2.8.

Conduction Band

E - 0

Electron Energy

Trap Ground State

A

SE

Figure 2.8 Energy diagram for an electron bound to a point charge in the presence of a uniform electric field (Poole-Frenkel effect) [21].

The Poole-Frenkel effect leads to a decrease in the potential barrier ET

by an amount 8E given by

8E = 13-if (2.6)

23

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where 13 is the Poole-Frenkel constant and F is the applied electric field.

Equation 2.4 must be modified to take this barrier reduction into account

and it becomes

1 I- ET -13,51, zR

= vpllext kT j

2,6 Summary

(2.7)

In this chapter, the physical structure and properties of amorphous

selenium were introduced. Studies have shown that atoms in amorphous

selenium exist in a twofold coordinated chain structure. The dihedral angle

of this chain remains constant in magnitude but changes sign in a random

fashion. Thermally derived defects in the chain (VAPs) also exist in the

amorphous state.

Further, it was shown that the disordered structure of amorphous

materials, such as selenium, leads to a different band model than for

crystalline materials. The disorder in amorphous solids is thought to give

rise to states, localized in space, in the mobility gap of these materials. In

amorphous selenium, the VAP structures are the origins of the localized

states. Theses band structures in turn govern the optoelectronic properties

of amorphous selenium.

The absorption coefficient of a-Se is dependent on the photon energy

of the incident light. The optical gap in amorphous selenium is —2.05 eV,

and photons with lower energy will experience little or no absorption. The

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quantum efficiency of a-Se is dependent on both the energy of the incident

photons and the applied electric field. The field dependence of the quantum

efficiency has been explained by the Onsanger theory, and it only reaches an

acceptable level at high electric fields and photon energies larger than the

optical gap.

Charge transport in amorphous materials can occur through a variety

of processes. Charge transport studies on amorphous selenium have

suggested that a diffusive type transport in the extended states near the

mobility edge is the dominant process for transport. However, this transport

is further modulated by the existence of shallow traps near the mobility

edge. This reduces the mobility of the charge carriers through trapping and

release events from these shallow traps.

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3. TIME-OF-FLIGHT AND AMBIPOLAR

RECOMBINATION EXPERIMENTS

3.1 Introduction

Due to their disordered structure, the charge transport properties of

amorphous materials are difficult to model and understand mathematically.

With the use of quantum mechanics, crystalline materials are easily

understood since their long-range order greatly simplifies the mathematical

models involved.

The study of amorphous materials, then, relies heavily on empirical

measurements of the physical and electronic properties of interest. The

Time-of-Flight (TOF) transient photoconductivity experiment provides an

excellent means to study the charge transport properties of low mobility

materials. The principles of this technique will be introduced in this

chapter. The following section will present an analytical framework for

interpreting the resultant TOF waveforms for a material with a single

species of deep traps.

26

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3.2 Principles of the Time-of-Flight (TOF) Technique

The Time-of-Flight (TOF) transient photoconductivity experiment

consists of measuring the transient response that occurs due to the drift of

injected charge carriers across a low mobility solid. A simplified schematic

diagram of the TOF experiment is shown in Figure 3.1(a). A thin film, of

thickness L, of the material to be studied is sandwiched between two metal

electrodes, A and B. The top electrode A is connected to a high voltage bias

source Vo which sets up a uniform electric field across the sample. The

bottom electrode B is connected to ground through a sampling resistor R. It

is assumed that, for the present discussion, electrode A is kept at a positive

potential with respect to ground. A thin sheet of free carriers is injected into

the sample through some form of external excitation, and these carriers drift

across the sample under the influence of the applied electric field.

The analysis of the signal is greatly simplified when the absorption

depth 8 of the excitation is much less than the sample thickness L. This

ensures that bulk generation of carriers across the sample does not occur

and that only one type of charge carrier is swept across the sample. This

discussion thus assumes that electrons will be quickly removed from the

sample by the positive potential at electrode A while holes will drift towards

electrode B.

It is also important to ensure that the duration of the excitation tex is

much less than the transit time tT of the carriers. tex determines the initial

width of the charge carrier sheet that will cross the sample. This sheet is

used as a probe to examine charge transport across the thickness of the

27

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sample and its width will determine the spatial resolution of these

measurements.

Carrier Injection tex

T ----F 1

w . i ...+. . .±.±..+.+._+±.-11..+.± +.±

F2

1P h

iP

. (a)

(b)

x =0

x=x'

x = L

Figure 3.1 (a) Simplified schematic and (b) small signal ac equivalent circuit for the Time-of-Flight transient photoconductivity technique, where Cs is the sample capacitance.

28

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Time-of-flight measurements require that the dielectric relaxation

time, trei, of the material under study be much longer than the transit time

of the carriers. trei represents the time for the extrinsic charge carriers in a

material to decay to their thermal equilibrium number. TOF measurements

rely on the fact that the excess photoinjected carriers are not neutralized by

intrinsic charge carriers while they are drifting across the sample. This can

be assumed to be true when trei » tT. High resistivity amorphous

semiconductors generally fall into this category since they contain few

mobile intrinsic charges at room temperature.

The carriers injected into the sample perturb the applied internal

electric field Fo. The fields F1, behind the charge sheet, and F2, in front of

the charge sheet, as shown in Figure 3.1(a) can be determined at any

position x. By using elementary electrostatics, Spear [22] has shown that

= Fo + Lepow(x

—1j, (3.1)

and that

F = F

+ ep ow x 2 0 e (3.2)

where F0=V0/L is the applied electric field, po is the concentration of injected

carriers (in this example holes) in the charge sheet, w is the width if the

sheet, and e is the dielectric permittivity of the sample. If the amount of

injected charge powA, where A is the area if injection, is kept small enough

so that epow/c « Fo, the internal field can be approximated as being uniform

Fo.F1=F2=Vo/L. This is the small signal condition, and it corresponds to

29

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Qo(injected) « VoCs, where Cs is the capacitance of the sample. This

condition limits the number of carriers that can be injected into the sample

for TOF studies. If the small signal condition is not maintained throughout

the experiment, the TOF analysis must be modified to take the space charge

perturbation of the electric field into account [23].

As a charge q drifts within the sample, a charge is induced to flow in

the external circuit. Consider Figure 3.2. The work done moving charge q a

distance dx is given by

dW=F•q•dx, (3.3)

where dW is the work done moving the charge and F is the field in which the

charge is moving. The energy required to do this work must be supplied by

the external source and it is given by

dE = Vo • clQ. (3.4)

dx

dQ

Figure 3.2 The motion of charge q through dx induces charge dQ to flow through the external circuit.

30

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Equations 3.3 and 3.4 must be equal to each other according to the

first law of thermodynamics. The following equation can then be written

dQ = qdx L •

(3.5)

Equation 3.5 is known as Ramo's theorem [24]. In practical terms this

shows that the signal measured in the external circuit is due to an injected

charge moving through the sample from electrode A to electrode B. It

follows simply from Equation 3.5 that for a trap free solid, the induced

photocurrent through the sampling resistor is

i ph (t)

ePot,

for t < t,

0 for t t,

(3.6)

Equation 3.6 is valid for both holes and electrons by substituting no for po.

There are essentially two methods of measuring the induced charge

that flows in the external circuit. Figure 3.1(b) shows the small signal ac

equivalent for the circuit in Figure 3.1(a). The induced photocurrent iph(t) in

this circuit must flow through the parallel RC circuit. Let V(s) and Iph(S) be

the Laplace transforms of the voltage signal and photocurrent. For the

circuit shown in Figure 3.1(b), they are related through

31

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V(s) — sRCs + 1

IPh

(s). (3.7)

The bandwidth of the measured signal is arbitrarily defined as the

reciprocal of the carrier transit time tT.

The first measurement involves measuring the current pulse

produced by the drifting charge sheet. If RCs«tT then the inverse Laplace

transform of Equation 3.7 leads to

v(t) = Ri ph (t) for RC < tT (3.8)

Equation 3.8 is the so-called I-mode signal because the observed output

signal is directly proportional to the photocurrent. In a trap-free solid, the I-

mode signal rises instantaneously to a constant level when the charge

carriers are first injected and remains so until the charge sheet reaches the

opposite electrode when the signal falls to zero.

The second technique relies on integrating the induced charge Q that

moves through the sampling resistor. Again consider Equation 3.7, but with

RCs»ti, for this case. Taking the inverse Laplace transform gives a signal

ri v(t)=--

Cs j°iP h (t)dt for RCs » tT (3.9)

Equation 3.9 represents the V-mode signal. The V-mode signal is the

integral of the I-mode signal. As such, it will rise in a linear fashion after

32

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the charge carriers are injected until they drift across the sample at which

time the signal will flatten and remain constant.

The I-mode and V-mode signals are modified by interactions with the

deep traps that can occur in the mobility gap of amorphous semiconductors.

Deep traps are localized states that exist deep within the mobility gap.

Release times from the deep traps are very long due to the large potential

barrier that carriers must be thermally excited over. These traps can

significantly reduce the concentration of free carriers in the charge sheet as

they drift across the sample. For a given species of trap, characterized by a

mean trapping lifetime 'cc and a release such that carrier release is

insignificant during tr, the number of free carriers will be diminished in an

exponential manner. The photocurrent in Equation 3.6 is then modified as

ePo r t 1 tT

expi — I for t < tTL "Cc J

i ph (t)

0 for t tT

(3.10)

to account for the decrease in the concentration of free carriers. The

resulting I-mode signal is given by

v(t) =

Re Po .r xpl

tT L

0

t I for t < tT— —

j

for t ?_ tT

(3.11)

33

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The resulting V-mode signal can be found by integrating the photocurrent

signal according to Equation 3.9. This yields

ePot t 1—ex ---- for t < tT

Cs tT 'CC v(t) =

ePot r CS tT

exp I for t tTt c

(3.12)

A comparison of the trap free and deep trapping signals for I-mode and V-

mode signals is shown in Figure 3.3.

v(t)A v(t)A

t=0 t=t T

(a) v(t)A v(t)A

z I I

t4) t=t T t

(C)

t=t

0:0)

I t=0 t=t T t

(d)

Figure 3.3 Signals from the TOF experiment where (a) and (b) are I-mode signals for the trap free and deep trapping only case and (c) and (d) are V-mode signals for the same cases [20].

34

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There are advantages and disadvantages inherent with both the I-

mode and V-mode techniques. For example, I-mode signals readily lend

themselves to the determination of carrier transit times since an abrupt

change in signal magnitude is evident when the carriers exit the sample at

the opposite electrode. V-mode analysis on the other hand can be used to

determine the total amount of charge injected into the sample. Equation

3.12 has also been used to estimate the trapping time of carriers into deep

traps [51].

3.3 Transient Trap Limited Theory

The previous section developed the principles of the TOF experiment.

In this section, a transient trap-limited theory will be developed for trapping

and release from a single set of monoenergetic traps within the mobility gap

of an amorphous solid.

Figure 3.4 represents some semiconducting material. Consider a thin

slice of the material with a thickness dx. If a current due to an electron

charge packet is flowing in the material, the number of electrons in the slice

may increase due to the net flow of electrons into the slice or due to the net

thermal release of trapped electrons within the slice. Recombination effects

may be ignored because only one type of carrier is present in the sample.

This situation can be expressed by the continuity equation as

on(x, t) 1 8J(x, t) SnT (x,t) St e Sx St

35

(3.13)

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where n(x,t) is the concentration of free electrons in the sample, J(x,t) is the

net current density flowing into the slice, and nT(x,t) is the density of

trapped electrons in the slice.

x+dx

J(x,t) ►J(x+dx,t)

tc

Figure 3.4 Current flow with trapping and release processes in a thin slice of thickness dx.

There are two components which make up J(x,t). The first component

consists of the drift of electrons under the influence of the applied field.

This is expressed as Jc(x,t)=epon(x,t)F(x,t) where e is the electronic charge,

go is the mobility, and F(x,t) is the electric field. The second component is

due to spatial variations in the concentration of charge carriers and is given

by Jp(x,t)=eD8n(x,t)/Sx where D is the diffusion coefficient. The net current

density is therefore given by

J(x, t) = egon(x, t)F(x, t) + eD Sx •

8n(x, t) (3.14)

The substitution of Equation 3.14 into Equation 3.13 leads to the one

dimensional continuity equation for electrons given by

36

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on(x, t) on(x, 45F(x, 0 52 n(x, t) OnT (x,

St oxµ0F(x, + on(x, t) 8x + D 53(2 — St . (3.15)

The expression for SnT(x,t)/8t, known as the rate equation, is

determined by the difference in the instantaneous trapping and release

rates. Given tc and TR as the capture and release times, the rate equation is

SnT (x, t) n(x, t) nT (x, t) St T 'CR

(3.16)

A number of simplifying assumptions can be made to allow for the

simultaneous solution of Equations 3.15 and 3.16. For example, the internal

electric field for small signal TOF measurements is assumed to be uniform.

This means that the 8F(x,t)/5x term may be neglected. The diffusion term

may also be neglected since the magnitude of the diffusion current term is

usually considerably less than the conduction current.

The following initial conditions are required to solve Equations 3.15

and 3.16 simultaneously

and

n(x,0) = NoS(x,0), (3.17)

nT (x,0) = 0 for x > O. (3.18)

These conditions correspond to an impulse of No electrons being injected into

the sample at time t=0 and position x=0. Boundary conditions which take

into account the finite length of the sample must also be used. These are

37

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n(x,t)= 0 for x > L, (3.19)

and

nT(x,t)=0 for x>L. (3.20)

Equations 3.15 and 3.16 have been solved by applying these initial

and boundary conditions and by using Laplace transform techniques[251.

This provides an expression for the free electron charge density given by

No I- z 1 No z (t — z)lj (4) 2(t — z)

n(x, — exit i:

— 71SO — z) + 110F ex rcc U(t — z) , (3.21)

where z=x410F, Ii(4) is the hyperbolic Bessel function, U(x) is the unit step

function and 4= (2Vorcz(t— /TR ) itc

Equation 3.21 consists of two components. The first term represents

the charge that remains in the injected packet as it drifts across the sample.

These carriers do not undergo any delay due to trapping and release events

but the number of these untrapped charges does decrease exponentially as

exp(-t/tc) until they reach the opposite side of the sample. The second term

represents those carriers that have been trapped out of the charge packet

and are released back into the conduction band at time t. These carriers will

lag behind the untrapped carriers, due to at least one trapping and release

event, and contribute to the signal at times greater than t=I4toF where go is

the microscopic mobility.

38

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The time dependence for the free carriers in the sample can be found

by integrating Equation 3.21 over the length of the sample. However, the

detrapped portion of Equation 3.21 cannot be integrated to give a closed

form for N(t), so limiting or particular cases are used to evaluate the

trapping parameters. These special cases do not pose a problem for

predicting the transient response of charge carriers during TOF experiments

since they can be obtained by making appropriate choices as to sample

thickness, bias voltage, and temperature.

3.3.1 TC«'CR<tT Case

The conditions tc«tT<TR state that the capture time is much shorter

than the time it takes for the fastest carriers to cross the sample determined

by tT=L/µ0F, and that Tx is comparable to tT. These conditions imply that the

carriers will undergo many trapping and release events, from a shallow

species of traps very near to the conduction band edge, before they complete

their transit across the sample. Imposing these restrictions on Equations

3.15 and 3.16 causes the time derivative of the total charge in the conduction

band to vanish over a long time interval. By making use of the principle of

conservation of charge, the total number of free charges in the conduction

band is given by

N = No T c •

'Lc + TR (3.22)

The resulting I-mode photocurrent signal can be found by substituting

Equation 3.22 into Equation 3.6. This expression is

39

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eNo Tc tc +TR 'ph for tic < t < tT • (3.23)

tT Tc +TR Tc

This resembles the trap free I-mode case except that the transit time tT has

been increased by a factor of erci-tx)itc. This in turn implies a reduction in

carrier mobility from .to to µ, given by

tc = 011o

t + C TR (3.24)

where the scalar 0 is referred to as the shallow trap-controlled transport

factor. When the mobility of the carriers is reduced by the time spent in the

traps, the transport mechanism is known as shallow trap-controlled

transport.

3.3.2 High Field Case (tT<Tc)

When the applied electric field is sufficiently high, it is possible that

charge carriers will cross the sample without becoming trapped and that the

equilibrium between trapping and release events found in the previous case

will not be reached. The photocurrent signal for this case can be separated

into two terms. The first term represents the drift of carriers in the charge

sheet for t<tT. This current signal has been derived as [21]

eN0 r TR tic +TR t)

I for t < tT. i ph ( t ) I L exp — (3.25) tT ctic +TR t c +TR t ct it

40

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If detrapping is neglected by letting TR—>co, then Equation 3.25 reduces to the

simple case of deep trapping only i.e. Equation 3.25 reduces to Equation

3.10.

The second term, for t>tT, represents the response for those carriers

that were trapped and then later released back into the conduction band.

Most of these carriers finish crossing the sample without being trapped

again. The current signal for this case has been derived as[211

eN0 tT p[ t iph (0 =

2 Tctiz ex

'CR

3.4 Summary

for t > tT. (3.26)

The principle of the Time-of-Flight experiment and the transient

response expected for a single species of trap have been introduced in this

chapter. The TOF technique is a powerful method for studying charge

transport in amorphous and low mobility semiconductors. There are

essentially four conditions that must be maintained throughout the TOF

experiment. These are:

1. The absorption depth, 6, of the charge carriers must be much less than the thickness of the sample (8«L).

2. The duration of the injection pulse, tex, must be much shorter than the transit time of the carriers across the sample (tex<<tT).

3. The dielectric relaxation time, trel, must be much longer than the transit time of the carriers (trei»tT).

41

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4. Small signal conditions must be maintained throughout the sample (Qo(injecthd)«CsVo).

Furthermore, there are two methods for measuring the charges that

flow in the external circuit during the TOF experiment. These are the I-

mode and V-mode measurements. Each of these techniques has its own

advantages, and the use of one or the other depends on the parameter of

interest in the experiment.

The effect of the many trapping and release events found with a set of

energetically shallow traps is to reduce the mobility of the carriers because

of the time that the carriers spend in the traps. However, for a deeper set of

traps, the photocurrent signal will decay exponentially with a characteristic

trapping lifetime Tc.

42

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4. EXPERIMENTAL PROCEDURE

4.1 Introduction

This chapter describes the systems that were used to obtain

experimental data during the course of this work. It consists of three parts.

The first describes the procedures used for fabricating the samples. Next, a

review of previous recombination experiments is conducted before the

present Ambipolar Time-of-Flight (TOF)/recombination measurement

system is introduced. The final section gives a brief overview of the

Interrupted-Field TOF (IFTOF) method used for obtaining the trapping

lifetimes of carriers in Cl doped a-Se:0.2%As films of this work.

4.2 Sample Preparation

The stabilized a-Se alloy films were prepared by conventional vacuum

evaporation onto aluminum substrates. The polymer film used to protect the

Al sheet was first removed by ultrasonic cleaning in a sequence of acetone,

distilled water, methanol, and distilled water baths. The substrate was then

placed in a heated mixture (65 C) of sodium carbonate, sodium phosphate

and distilled water (caustic etch solution) to partially remove the oxide layer

on the surface of the Al substrate. The final cleaning sequence consisted of

the sample being dipped into a nitric acid solution and then washed in

43

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repeated cycles of distilled water and detergent solutions. The oxide layer

was regrown on the substrate by placing it in a 300° C furnace for 4-5 hours.

The oxide layer serves two functions. First, it acts as an insulator between

the substrate and selenium film to prevent charge carrier injection from the

electrode into the film [26]. Second, it provides an amorphous base onto

which the film can be deposited. The Al substrate was loaded into the

vacuum deposition chamber and heated to a temperature of 55° -65 ° C by

the substrate heater as described below.

The source material for the a-Se films were xerographic grade, liquid

quenched, vitreous selenium pellets obtained from Noranda Technology

Center, Pointe Claire, Quebec. The purity and chemical contents of the

pellets were verified by the supplier using optical emission spectroscopy.

The purity of the pellets was found to be 99.999%.

A NRC 3117 vacuum deposition system, shown in Figure 4.1, was

used to fabricate the a-Se films. The evaporation chamber was evacuated by

a diffusion pump until a pressure of —10-6 Torr was obtained. The Al

substrate was heated and maintained at a temperature above the glass

transition temperature for a-Se in order to produce films with good charge

transport properties [27]. The selenium pellets were contained in an open

stainless steel boat. A large ac current (100-150 A) was passed through the

boat to heat the pellets. The temperature was maintained at 270° C by

controlling the amount of current through the boat. At this temperature, a

deposition rate of about 2µm/minute was obtained. The substrate and boat

heaters were turned off when deposition was completed and the samples

were allowed to cool slowly before air was let back into the vacuum chamber.

44

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The completed films were then allowed to age in the dark, at room

temperature, for a period of 2-3 weeks to allow their physical properties to

stabilize. Samples used for recombination measurements were peeled off

from the Al substrate so that both sides of the film were available for

illumination.

Reflector

T/C Substrate Heater Substrate

Quartz X-tal

T/C

1

_IShutter

• Se enium

tainless Steel Boat

Rotation 4— Platform

150A

Stainless Steel Base

11F Diffusion Pump

Gas

Figure 4.1 Schematic diagram of the vacuum deposition system.

In order to facilitate the TOF/recombination measurements, semi-

transparent Au electrodes were deposited on the samples. The deposition

was carried out in a Hummer VI sputtering system, shown schematically in

Figure 4.2. The sample was loaded into the sputtering chamber of the

Hummer VI which was then evacuated and flushed with argon until a

pressure of 70 millitorr was obtained. A large dc bias voltage (3000V) was

45

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applied between the anode and cathode causing the Ar within the chamber

to ionize and form a plasma. The positively charged Ar ions were

accelerated towards the cathode where the Au target was located. The ions

dislodged Au atoms from the surface of the of the target which were

dispersed throughout the chamber and settle on the sample. Masks were

used to define the areas on the sample where the Au was to be deposited.

Cathode Shield

Substrate

Insulator

High Voltage

Argon ions Electrons

4, 4i

Cathode Vacuum ie.„—Chamber Target

Vacuum Pump

Anode

i3) Needle Valve

Argon

Figure 4.2 Schematic diagram of sputtering system.

In the present study, electrodes where sputtered on each side of the

sample so that each could be illuminated. The region outside of the

sputtered electrodes were masked with PVC electrical tape to prevent

photogeneration of carriers in the fringing fields during TP measurements.

The sputtered samples were then mounted onto cardboard backing and

46

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electrical connections were made by attaching wires to the electrodes with

highly conductive silver paint.

4.3 Ambipolar Time-Of-Flight (TOF) Apparatus

Time-of-Flight transient photoconductivity (TOF-TP) experiments

were pioneered in the 1950s and 1960s by Brown [28], Spear [20], and

Kepler [29]. They were able to apply the technique to the study of a wide

variety of materials. The power of this experiment is that it allows for direct

measurement of charge carrier mobility. A simplified schematic of the TOF

experiment is shown in Figure 4.3.

The TOF experiment consists of measuring the transient photocurrent

that results when photoinjected charge carriers drift across a

semiconductor or insulator. The most common method of injecting charge

carriers into the sample is a short duration light pulse. The spectral

components of the light pulse must be matched to the energy gap of the

material being studied so that bulk generation of charges does not occur due

to weakly absorbed light components. A number of different sources have

been used to study different materials, and these include xenon flash

lamps[30], N2 flash lamps[31], nitrogen pumped dye lasers[32], and Q

switched ruby lasers[33].

47

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Current

tc Time

Output

Figure 4.3 Generalized schematic of TOF experiment.

Variations on the TOF experiment have also been reported. These

include the use of different bias schemes (dc or pulsed bias). Advanced

application of the bias has been used to study the effect of negative bulk

charge on the charge transport properties in the sample[34]. Charge carrier

surface recombination has been examined by delaying the application of the

bias until after the carriers have been photoinjected. This allows the

carriers to interact before they are swept apart by the bias field[35].

A double photoinjection TOF technique was used by Dolezalek and

Spear[36] to study bulk recombination in orthorhombic sulphur crystals.

This experiment involved the photoinjection of one species of carrier followed

by a second injection, on the other side of the sample, of carriers of the

opposite sign. The carriers underwent recombination as the charge packets

drifted through each other. This was evidenced by a reduction in the total

48

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photocurrent observed. The recombination experiment performed in the

course of this study is based on the technique used by Dolezalek and Spear.

A schematic of the ambipolar TOF apparatus used was shown

diagrammatically in Figure 4.4. A high voltage bias, V, was applied to the

sample which is grounded through a sampling resistor, RSAMPLE. Following

the application of the bias voltage, mobile charge carriers were photoinjected

into the sample, by the laser only, where they drifted across the sample and

induced a current in the external circuit. The transient current through

RSAMPLE was then measured.

In order to perform the recombination experiment, a second

photoexcitation source was required. This source was used to inject charge

carriers of the opposite sign into the other side of the sample. The xenon

flash was triggered and a negative charge packet was photoinjected into the

sample. While the negative charge packet is drifting towards the positive

electrode, the laser was triggered and injected a positive charge packet

which started to drift towards the negative electrode. The oppositely

charged carriers drifted towards each other and underwent recombination as

the respective charge packets passed through each other. The

recombination event was witnessed by the decay in the external

photocurrent through the sampling resistor.

49

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Fiber

tX ENON 'LASER

-Se

Diffuser 4-0-;

r-11 Pulse Bias Circuit

A

SAMPLE

•—g•

Xenon Flash

2

Trigger Signal Generator

CCD Camera O o O 0

U000 000 000

0000 0 0

0 0 0 0

tosc t:1-1- 10.

0 0 0 a a o 0000

0 0

Oscilloscope

Figure 4.4 Diagrammatic view of ambipolar TOF experiment apparatus.

4.3.1 Photoexcitation Sources

Injection of transient charges was accomplished through the use of

optical excitation. Both a xenon flash bulb and a nitrogen laser were used

as photoexcitation sources. The spectral outputs of these sources were

appropriate for use with TP measurements in a-Se alloys.

4.3.1.1 Xenon Flash Bulb Source

The xenon flash source made use of short arc length (1.5 mm) xenon

flash bulbs manufactured by EG&G and Hammamatsu as quiet xenon flash

50

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bulbs. The circuit used for obtaining short duration light pulses from the

xenon bulbs is shown in Figure 4.5. The high voltage capacitor, CH, was

connected across the electrodes of the xenon flash bulb. This capacitor was

charged up to 1600V. A pulse transformer was connected to trigger probes

in flash bulb. Capacitor CT was connected in series with a silicon controlled

rectifier (SCR) to the primary of the pulse transformer and was charged to a

voltage of 170V. When the SCR was triggered by the triggering circuit, CT

was discharged through the pulse transformer and a high voltage spike (5-7

kV) was applied to the trigger probes of the xenon flash bulb. The high

voltage spike caused the xenon gas in the spark gap of the flash bulb to

ionize, which in turn lowered the impedance of the spark gap. When the

impedance in the gap had been lowered sufficiently, CH discharged through

the spark gap providing the light pulse. The light from the xenon flash bulb

was passed through a CuSO4 solution filter to remove the undesirable red

wavelengths. These wavelengths would have resulted in bulk generation of

carriers in the samples. The xenon flash bulb circuitry was contained within

well grounded shielding, and RF filters and optocouplers were used to

prevent high-frequency transients from feeding back into the measurement

systems.

The output pulse from the xenon flash circuit was measured with the

reverse biased p-i-n photodiode circuit shown in Figure 4.6(a). The width of

the light pulse, which is shown in Fig 4.6(b), was —140ns at the half power

point. This is much shorter than the typical transit times experienced with

amorphous chalcogenide semiconductors.

51

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CuS

O4

SO

LUT

ION

PA

RA

BO

LIC

R

EF

LEC

TO

R

H V

4- NV

LV

TRIG

GE

R

INP

UT

LV

Fig

ure

4.5

S

chem

atic

sk

etch

of

xeno

n fl

ash c

ircu

it.

Page 65: CHARGE CARRIER RECOMBINATION IN AMORPHOUS SELENIUM …

Oscilloscope

47

a)

p-i-n Diode (S1722-02)

33n

b)

Figure 4.6 a) Reverse biased p-i-n measurement circuit. b) Light output Vs time for xenon flash. Horizontal axis: 200ns/div.; Vertical axis: 20mV/div.

4.3.1.2 Nitrogen Laser Source

The second photoexcitation source was a Laser Photonics LN 103 C

transversely excited atmospheric (TEA) nitrogen (N2) laser. This laser was

capable of providing a 250kW peak power output pulse with a duration of

300 ps at a wavelength of 337.1 Tim.

53

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The TEA N2 laser is a 3-level laser system where the laser transitions

occur between the C31Iu (C-state) and the B31Ig (B-state) electronic states in

the N2 molecule, shown in Fig 4.7[37,38]. Electrons are excited from the

ground state to the C-state by impact collisions with external electrons. The

electron lifetime at the C-state is relatively short (-2ns) at atmospheric

pressures, while the B-state is metastable. Therefore cw operation is not

possible and TEA N2 lasers may only operate in a pulsed mode. In order to

achieve population inversion between the C-state and B-state, a very rapid

excitation method is required, in this case, a very fast electrical discharge.

2 15

flu

10

E(eV)

Electron Collision

1.0 2.0 Nuclear Seperation (A)

3.0

Figure 4.7 Potential energy curves for lowest triplet states in N2

molecule [37].

Figure 4.8 shows a simplified schematic circuit for the excitation of a

TEA N2 laser. This circuit makes use of the Blumlein excitation method.

Initially Ci and C2 are charged to the high voltage (HV) potential (10-20kV).

The electrodes in the laser channel are effectively shorted by an inductive

lead. When the spark gap is triggered, Ci is rapidly discharged through the

54

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gap. The inductance in the loop is such that a damped oscillation occurs in

the circuit, and a voltage reversal appears on Ci. This causes an overvoltage

and electrical breakdown in the laser channel. With the electric field

transverse to the electrodes, the discharge is so fast that atmosphere glow

discharge and laser action occur on the order of 10-9s.

HV

Trg.

Spark Gap

TLaser Head

C2

Figure 4.8 Blumlein circuit used for rapid excitation of N2 laser.

The LN 103 C laser is triggered by two separate I IL pulses. An

initial pulse of at least 100ns duration must be applied to the Trigger Reg

input of the laser in order to charge it. A second pulse of at least 100ns

duration must be applied to the Trigger Low input, between 30 and 50 i.t.s

later, to fire the laser. If the second pulse does not occur within 50 i.ts, the

laser will self-fire. Figure 4.9 shows the timing requirements to fire the

laser.

55

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4- 10011S

+5V

Laser Self Fires

Triggering Window

Trigger Reg

Trigger Low

—mot 4-- 100ns

+5V

0 us 30 us 50 us

Figure 4.9 Triggering requirements for the LN 103 C N2 laser.

4.3.2 Timing Signal Generator

A TTL timing signal generator was used to provide the required

timing control signals for the TP experiments performed

(TOF/Recombination as well as the IFTOF measurements to be discussed

later). The timing signal generator made use of TTL 74123 monostable

multivibrators and TTL 7476 J-K flip flops to produce the control signals

X2, Xi, and Xh which are shown in Figure 4.10. A schematic of the timing

generator is shown in Figure 4.11.

Signal Xi controls the application of the bias voltage used in the TOF/

Recombination experiment. X2 deactivates the amplifier protection circuitry

after the RC transients, created by switching the bias voltage across the

sample, died out. When the measurements are complete, X2 reactivates the

amplifier protection circuitry before the bias voltage is removed by Xi. The

Xd signal is used as a trigger for a set of digital delays that control the

56

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triggering of the oscilloscope and photoexcitation source used in the TOF

experiment. The oscilloscope is triggered slightly before the photoexcitation

source so that the baseline is visible before the TP waveform is viewed. In

the recombination experiment, where two photoexcitation sources are used,

the digital delays are used to ensure that the two sources are not triggered

at the same instant, i.e. so that the oppositely charged carriers are not

injected into the sample at the same time. Finally, the signal Xh is used in

the IFTOF experiment. This signal controls the application of the switched

bias source used for IFTOF measurements. The details of the timing

requirements for the IFTOF experiment will be discussed later.

2.2ms 2.2ms

4— 2.2 ms

tic =3.5 - 75 us

t4 =tlaser

-0' t D1

T2

tosc t=0 for IFTOF Time

X h

Figure 4.10 Timing signals from Timing Signal Generator. tND, ATi, AT2, and AT3 are adjustable as shown in Figure 4.11.

57

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5V

4K7 4K

lop'-

11

B

CLR

0 >

1,

R/C

us

C

0 3

0

A

5V

OK

K

-i---141-1-4 5V

20K

K

20K

K

95

V

03V

Qsv

B

CLR

R/C

ti

c T

3 5-

A

3

22K

.2 70r

A

CLR

B

A

0

5V

0

4K

7

lOp

r

3

AB

CLR

0 3

a/c

r:

0

A

B

CLR

R/C

CQ

T2

0A

A

—C

r-T

T"

lOa

r IA

, Igo

r

B

CLR

0 3

+

••4

R/C

1

.1

C

AT

I 53

A

AB

CLR

0

4K

7

...a 1

0p

r a/c

ft 1.0

5V

(ii‘r

0

CLR

4K

7 10p

r R

/C

a.

C

B

7

B

CLR

0

R/C

Ft;

A

3-6

3-

3

o]

Y

3

05V

CLR

0 3

R/C

-C

-C

.IK7

A

3V

A B

CLR

0 3

-

R/C

W

C

A B

07

SE

1

J

0

C C

LK

CK

o

CLR

0 5V

••••••••-‹

c —

C

5V

ASE

TJ

0

cLK

K

0

CLR

>—

=1

x 1

a--

--"D

X2

3

7K5

in,

B

C C

LR

R/C

tiA

a 5 a

B

CLR

2

R/C

I.J

C c

.27)." A

V

D.

3

Q3V

fa--C

ASE

T 0

C C

LK

O•

CK

0

cia

3

3

Fig

ure

4.1

1 C

ircuit

dia

gra

m

for TT

L trig

ger sig

nal g

enerato

r.

D)

v

0 X

Page 71: CHARGE CARRIER RECOMBINATION IN AMORPHOUS SELENIUM …

4.3.3 Digital Delays

The timing delays required for triggering the oscilloscope and

photoexcitation sources were provided by Berkeley Nucleonics Corporation

(BNC) Model 7010 and 7065 Digital Delay Generators (DDG).

The Model 7010 DDG consists of two count chains and various other

support circuits. The first count chain is used to develop the time base

signal that determines the resolution of the DDG. The resolution of the

Model 7010 varies from 0.1 µs to 1 ms giving a range from 0.1 la to 99.999 s.

The second count chain uses the time base signal from the first count chain

to generate the delay signal. The support circuits are used for control

operations, pulse shaping, and other functions as needed.

The Model 7065 DDG operates in a manner very similar to the Model

7010. The major differences between the two units are their resolution and

range. The Model 7065 has a resolution of 1 ns and a range from 1 ns to

999.999 gs.

4.3.4 Bias Application Circuit

A pulsed bias circuit, shown in Figure 4.12, was used to prevent the

build up of bulk space charge in the sample during the time that the bias

voltage is applied in the TOF/Recombination experiment. The bias voltage

was supplied by an EG&G Ortec 556 high voltage supply. The output

voltage from the supply was switched across the sample by a SPST reed

59

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relay (EAC 061AY*050CAA). The coil of the relay was energized by the

collector current of a 2N3904 BJT. A 1N914 diode and a capacitor were used

to protect the BJT from an overvoltage state when the current through the

relay coil was interrupted. The pulse bias circuit was well shielded and was

further isolated from the experiment control circuitry by use of a HCPL-2601

opto-isolator on the trigger input. This was done in an attempt to reduce the

feedback of transients into the TOF/Recombination system. The circuit was

activated by a standard TTL pulse applied to the Trigger In input.

9V I --11011F

270 5.6k

HPCL-2601 2N3904 lk

1.8k

1.5k

2N3904 1N914

OnF

High Reed Voltage Relay

In

Figure 4.12 Schematic of pulsed bias application circuit.

4.3.5 Voltage Follower Circuit

+5V

To Sample

The voltage follower circuit shown in Figure 4.13 was used to drive

the long BNC cables that were used to connect the sample and the sampling

resistor to the input terminal of the oscilloscope. A two-stage follower circuit

based on a 2N5484 JFET was used to provide a high input impedance so

that loading effects on the TP signal were minimized.

60

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A relay based protection circuit was incorporated to protect the

voltage follower from the large transient voltage that occured when the high

voltage bias was switched across the sample. The protection was provided

by a normally grounded SPDT relay (Potter & Brumfield JWD-172-1). The

relay was used to connect the sample and sampling resistor to the voltage

follower after the displacement currents had time to decay. The protection

relay was triggered by timing signal X2.

X2

4.7k

From () Sample

56pF 2N3904

1_

1N914 56

JWD-172-1

9 V 1100u_a_

T 12vT T 2N5484

1 M

2N2222A

—"Out

560

Figure 4.13 Schematic of voltage follower with protection relay.

4.3.6 Data Acquisition System

The TP waveforms were displayed on a Tektronix 2467B, 400 MHz

single shot bandwidth, analog oscilloscope. The waveforms where then

stored by making use of a DCS01 CCD Camera Data Acquisition System.

This system consists of a Tektronix C1002 charge-coupled-device (CCD)

camera, an IBM compatible PC DX01 video frame storage card, and the

DCS01 software for control and waveform manipulation. The data

acquisition system is shown in Figure 4.14.

61

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DXO1 Video Framtlag=g1=E1 Storage Board (in computer)

Panasonic Video Monitor

DCSO1GPH Software

Video Signal

Trigger

V

Computer

Tektronix 2465A/2467B Oscilloscope

0 0 0 0 0 0

00000 000 000 O 000 0 0

o 0 0 000

000000

0 0 0 n° Co° " 3° O o o 0

C1002 CCD Camera

Figure 4.14 Diagrammatic layout of data acquisition system. The system features include the C1002 CCD camera, Tektronix 2467B oscilloscope, an IBM compatible PC to house the frame storage board and run the DCS01 software, and the Panasonic VW-5350 video monitor.

The CCD camera was mounted to the front of the oscilloscope by an

adapter that blocked out external light. The imaging device in the camera

has a sensivity of 2 lux and consists of a planar pixel array. The dimensions

of this array are 490 pixels vertical by 284 pixels horizontal. Light from the

oscilloscope CRT is focused onto the imaging device and the camera converts

the light signal into a RS170 (NTSC) video signal. This video signal is then

passed to the DX01 frame storage board. In order to capture a waveform,

DCS01 software instructs the frame storage board to acquire the video

frame. The frame storage board then converts the captured frame into a 512

by 512 data point matrix which represents the target pixels. The light that

strikes each pixel is recorded in one of 256 gray scales. The DCS01 software

assumes a Guassian profile of the light distribution from the oscilloscope

CRT and from these determines the center of the beam trace. This finally

62

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results in a digitized waveform with a record length of 512 data points and a

vertical precision of 12 bits. The overall system accuracy is claimed to be at

least 99%.

The waveforms can be visually monitored on the Panasonic VW-5350

video monitor. The DXO1 frame storage board can pass the RS170 video

signal to any device that will accept it as a video input.

The DCS01 software is a menu driven data acquisition package that

is used to acquire and digitize the signal from the CCD camera. The

software provides calibration routines that can be used to correct for

systematic optical and linearity errors inherent with the camera/oscilloscope

combination. Waveform measurements such as rise and fall times,

frequency, and duty cycle are available as soon as the waveform is acquired.

DCS01 also contains built-in functions to perform numerical calculations

such as waveform addition or subtraction, and integration on acquired

waveforms. The data acquired with the DCS01 software may be stored in

either binary or ASCII formats. This allows for the export of data to other

software packages for further manipulation.

4.4 Interrupted Field Time-of-Flieht (IFTOF) Apparatus

The charge carrier deep trapping lifetime, t, in high resistivity solids

has been measured conventionally by looking at the exponential decay et of

the standard TOF waveform. This method failed with many materials

however because they exhibited a non-exponential decay. This may be

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attributed to factors such as space charge build up effects, Poole-Frenkel

barrier reduction effects, or sample inhomogeneity effects. This method also

fails with materials that have long deep trapping lifetime with respect to the

carrier transit time. In these specimens, the TOF photocurrent waveform

does not display a significant decay while the carriers are crossing the

sample and the lifetime cannot be accurately determined.

These limitations in measuring the charge carrier lifetime can be

overcome by the Interrupted Field Time-of-Flight (IFTOF) technique. This

technique has been used successfully by Spear and co-workers to measure

the charge carrier lifetimes in orthorhombic sulphur crystals[39] and a-

Si:H[40] and by Kasap and co-workers in a-Se alloys [27, 41]. The IFTOF

technique involves interrupting the transit of charge carriers as they cross

the sample in the conventional TOF experiment by removing the applied

bias field at some time Ti. Following an interruption time t1, the field is

reapplied at T2=Ti+ti, and the remaining charge carriers are removed from

the sample. A comparison of the standard TOF experiment and the IFTOF

experiment is shown in Figure 4.15. Figure 4.15 (a) and (b) represent the

timing sequence for applying the bias voltage and the resulting photocurrent

waveform for the TOF experiment while Figure 4.15 (c) and (d) represent

those for the IFTOF case. The charge carriers drift a distance x=TiLitt

(where L is the thickness of the sample and tt is the carrier transit time) into

the sample before the bias is removed. The carriers interact with the deep

traps located at x during the interruption time ti. The number of carriers

that become trapped during ti will be reflected in the recovered photocurrent

signal at i(T2). If a single mean free carrier lifetime can be assigned to the

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v(t) photoexcitation

(a)

i(t) A

time

v(t) A

time (b)

photoexcitation

i(t) •

ti

po. T 2 time

(c)

time (d)

Figure 4.15 (a)Timing sequence for the application of bias voltage in TOF experiment and (b) the resulting photocurrent waveform. (c)The timing signal for the application of the bias in the IFTOF experiment and (d) the resulting IFTOF photocurrent signal.

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the bias voltage from on/off or off/on produces a large displacement current

signal which decays with the time constant RCs. The magnitude of the

signal could be several hundred volts depending on the bias voltage being

used. This signal is several orders of magnitude larger than the resulting

photocurrent signal and would make it unusable. The displacement current

signals may also be damaging to any electronics used in the detection of the

photocurrent signal. Therefore, some method must be used to eliminate the

displacement current signals to successfully make use of the IFTOF

technique.

HV Switch

Displacement Current Signal -300V

—300V

J -20mV

Photocurrent Signal

Figure 4.16 Large displacement current signals are produced when the high voltage bias is switched on and off. This signal must be eliminated for the IFTOF experiment to be successfully implemented.

A number of different methods have been previously used to

implement the IFTOF technique. A complementary bias technique has been

reported by Kasap and co-workers[41]. During the 1960s, Helfrich and

Mark [42] used a resistance ratio bridge and floating bias supply to

eliminate the displacement current effects in transient space-charge limited

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measurements. The major disadvantage with this technique is that only

half of the bias voltage appeared across the sample. This problem can be

overcome by making use of a Schering bridge network [43]. A diagrammatic

representation of the IFTOF experimental apparatus, based on the Schering

bridge network, is shown in Figure 4.17. The N2 laser source, trigger

generator, digital delays, and data acquisition system have been previously

discussed in Sections 4.3.1.1 to 4.3.1.3 and 4.3.1.6.

Laser

HV Switch

Xtrg A Xh

td

Fiber

a-Se

Trigger Signal Generator

td

CCD Camera

•0 . * *

• • 0 0 0 . 13000 COO 0013 . 0000 0 0

0 0 0 MI 0 0

• . .0 Oon

Oscilloscope

Figure 4.17 IFTOF experiment schematic based on the Schering bridge network.

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4.4.1 Schering Bridge Network

A schematic diagram of the Schering bridge and high voltage supply

is shown in Figure 4.18. Two nulling capacitors are required, CNS and CN1,

to eliminate the switching transients between points A and ground. The

floating high voltage supply introduces 'stray' capacitances to ground,

represented by Ci and C2, and these must be taken into account when

balancing the bridge. CI simply adds to CNs so that the balance condition is

C2-I-CNS=CS. CN1 is used to null C2.

Figure 4.18 Schematic of Schering bridge network used to implement displacement current signal free IFTOF measurements.

Good I-mode photocurrent waveforms are obtained by optimizing two

opposing conditions. The I-mode signal measured between the bridge output

and ground is given by vo(t)=R'i(t) where i(t) is the transient photocurrent

and R' is the effective sampling resistance given by R'=RN111/(2RN-FR1). The

optimum output is obtained when Ri is larger than RN which maximizes R'.

This condition must be balanced against the fact that for good I-mode

signals, the time constant of the circuit must be much less than tT so that

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the signal is not integrated. Laplace analysis of the bridge network,

including the addition of a capacitance CIN across Ri to account for the input

capacitance of the amplifier, relates Vo(s) and I(s) as follows

Vo (s) = [R7 (1 + sR'C')]I(s) (4.2)

where C'.2C1N+Cs+CNi is the effective integrating capacitance. Therefore, in

I-mode operation, the time constant, R'C', must be less than tT.

The variable components CN1, CN2, and RN are used to adjust the

bridge to an optimal balance condition. However, since the Schering bridge

is floating, it is very difficult to balance the bridge so that no displacement

current signal appears. The differences in the high frequency permittivity of

selenium and the ceramic capacitors used to null the bridge also creates

difficulties in balancing the bridge. In order to extract the photocurrent

signals, the following procedure had to be used. First, the bridge was

balanced to a point where the magnitudes of the displacement current and

photocurrent signals were similar. Next, two measurements were

performed, one with photoexcitation and one without. The two resulting

waveforms were acquired and digitally subtracted from each other using the

DCS01 software to provide a net displacement current free photocurrent

signal. This method has been used to extract displacement current free

photocurrent signals in photocurrent reversal measurements on a-Si:H films

[44].

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4.4.2 High Voltage TMOS Switch

The switching of the bias voltage was accomplished by making use of

two n-channel 1kV TMOS transistors in a totem pole configuration shown in

Figure 4.19. The high voltage source was provided by Eveready dry cell

batteries. The bias voltage is varied by simply changing batteries. The

gate-source voltage for switching each TMOS transistor is provided through

CMOS optocouplers (HCPL-2200) powered by floating 9V batteries. The

floating batteries were used because the maximum gate-source voltage the

TMOS transistors can sustain is ±20V. Common-emitter push-pull driver

circuits were added to the gates of the TMOS transistors to source and sink

gate charge as fast as possible. The switching time for this circuit is

approximately 150 ns. This switching time is considerably shorter than the

transit times encountered in this study.

— To Schering Bridge

Figure 4.19 Schematic of TMOS high voltage switch.

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The trigger signal for the high voltage switch is provided by the Xh

signal from the trigger signal generator discussed in Section 4.3.1.2. The

interruption time t1 is controlled by varying the RC combinations of the TTL

74123 monostable multivibrators used in the trigger signal generator.

4.5 Summary

In this chapter, a brief description of the sample preparation was

given. Following the thermal evaporation of a-Se alloy pellets onto Al

substrates, Au electrodes were sputtered onto the samples to facilitate

transient photoconductivity measurements.

A TOF transient photoconductivity apparatus was also described.

This apparatus allows the charge transport properties of high resistivity

solids to be examined. By adding a second photoexcitation source and an

extra digital delay, the TOF apparatus can be used to study bulk

recombination in these solids.

Finally, an IFTOF apparatus was introduced to study deep trapping

lifetimes in high resistivity solids. The technique presented allows bias

voltages of up to 1kV to be used.

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5 RESULTS AND DISCUSSION

5.1 Introduction

The previous chapter described the experimental details of the

ambipolar TOF and IFTOF measurement systems that were used during the

course of this work. This chapter presents the experimental results obtained

using these techniques on chlorinated a-Se:0.2%As electrophotographic films

suitable for x-ray electroradiography. Amorphous Se:0.2%As doped with Cl

is normally referred to as stabilized Se.

It is important to know the charge transport and deep trapping

properties of the materials being studied before performing the ambipolar

recombination experiment. Initially, conventional TOF measurements were

performed to study charge transport in the a-Se films. Next, IFTOF analysis

was used to provide information about the deep trapping that occurred in

the samples. Finally, the ambipolar TOF technique was used to analyze the

recombination effects in the films.

5.2 Charge Transport Study

The assumption that the internal field in the sample, set up by the

applied bias voltage, is uniform must be made in order to perform TOF

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analysis. When the small signal conditions are met, the field is negligibly

perturbed and remains constant. This is shown experimentally by the

almost rectangular shape of the photocurrent signals for a-Se samples with

long carrier lifetimes. This is the expected shape for a constant field and

drift mobility.

Tabak and Scharfe[45] have shown that the internal field will remain

constant and uniform following the bias application until a transition time

tsc is reached. The transition tithe for a-Se is typically on the order of 100

ms. After tsc, a bulk charge builds up within the sample, due to charge

injection from the contacts, and the field becomes non-uniform. This non-

uniformity may be determined from the Poisson equation dF/dx=p/e.

Photoexcitation in the measurements completed for this work took place a

few milliseconds after the application of the bias voltage to preclude these

field perturbations.

Repeated measurements may result in a build up of trapped bulk

charge in the a-Se film due to the trap release time being very long. This

trapped bulk charge will distort the applied field, again as determined by

the Poisson equation. This can be avoided by performing single shot

measurements and by dark resting the samples in a short circuit condition

between measurements to discharge any bulk charge.

Figures 5.1(a) and 5.1(b) shows the I-mode TOF waveforms for holes

and electrons respectively. The interaction between the drifting holes and

deep traps is minimal. This is evidenced by the lack of any decay in the top

of the hole photocurrent waveform. The electron waveform however, does

74

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show some exponential decay. The nature of this waveform can be described

by Equation 3.10 which is restated here in slightly different form as

Iph (t) = Ic, exp[--t ] for t < , (5.1)

where Io is the initial value of the photocurrent and ti is the carrier deep

trapping lifetime. The electron lifetime for this sample was estimated to be

Te.850 gs from this waveform.

tT

4

(a)

tT

12 Time (go 0 100 200 300

(b)

Time (i.ts)

Figure 5.1 I-mode TOF waveforms for a 195.1 gm a-Se:0.2%As film for (a) hole transit and (b) electron transit. The transit times are indicated by tT.

The relationship between the carrier mobility µ. and the measured

transit time tT is given by

LztTV ,

75

(5.2)

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20

15

10

5

0 0.000 0.001 0.002 0.003

1/Voltage (V-1)

0.004 0.005

Figure 5.2 TOF plot of transit time versus 1/voltage for holes in a-Se:0.2%As film showing j.th =0.125 cm2V-1s-1.

400

350

300

250

.1" 200

150

100

50

0 0.0000 0.0005 0.0010 0.0015 0.0020 0.0025 0.0030

1/Voltage (V-1)

0.0035

Figure 5.3 TOF plot of transit time versus 1/voltage for electrons in a-Se:0.2%As film showing ge=0.0034 cm2V-is-1.

76

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where L is the thickness of the film, and V is the applied bias voltage.

Figure 5.2 is a plot of tT versus V-1 from TOF transit time analysis for hole

transport The slope of the straight line yields a hole mobility of i.th = 0.125

cm2V-1s-1. Similarly, Figure 5.3 shows an electron mobility of lie = 0.0034

C1112V-IS-1 .

When the drift mobilities of both holes and electrons are calculated

using Equation 5.1 and plotted as a function of electric field, the behaviour

in Figure 5.4 is observed. The hole mobility shows no observable field

4

1.000

0.100

0.010

0.001 1.E+5 1.E+6

F(Vnr')

•gh

1.E+7

Figure 5.4 Plot of hole and electron mobility as a function of the applied electric field. The hole mobility shows no observable field dependence. The electron mobility shows a very slight field dependence of the form peocFo.o4.

77

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dependence. However, the electron mobility shows a very slight power law

field dependence of the type 1.1.eccF° where n was experimentally determined

to be n-0.04, which is very small. The exact nature of the electron mobility

field dependence is not yet fully understood. However, for the limited range

of fields used in this work, Ph and ge have both been considered field

independent.

5.3 Charge Trapping Study

The carrier mobility does not completely characterize the charge

transport process in semiconductors. As the carriers drift across the sample,

some of them become trapped in deep localized states within the mobility

gap. Release times from these deep traps is much longer than the release

times from the shallow, mobility controlling traps. This is due to the greater

potential barrier over which the carriers must be thermally excited.

The carrier lifetime ti can be used to provide a measure of how many

carriers are lost from the transport band through deep trapping. This is

extremely important to the recombination study described in the next

section where the trapping effect must be separated from recombination

alone.

The interrupted field time-of-flight experiment provides a means of

measuring the mean carrier lifetime by studying the fractional recovered

photocurrent as a function of interruption time. The measured photocurrent

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is directly proportional to the concentration of free charge carriers and their

drift mobility. The photocurrent is given by

iph (t) = en(t)µF, (5.3)

where n(t) is the concentration of free carriers and F=V/L is the internal

electric field, which is assumed to be constant (and uniform). As discussed

in the previous section, 11 is a material property and remains constant with

electric field. Measurement of the photocurrent at times ti and t2, just before

and after interruption, therefore provides a direct measure of the fraction of

recovered charge carriers since i(t2)/i(tl)=n(t2)/n(tl). For a single species of

deep traps with a well defined lifetime,

n(t i ) (t 2 — t i )] n(t2)

—ex —ti

(5.4)

Thus the slope of a semilogaritl-unic plot of i(t2)/i(ti) versus ti=t2-ti

gives the deep trapping lifetime. Charge carrier trapping occurs under the

zero-applied field condition, during ti, when using the IFTOF technique. As

such, the lifetime measured when using IFTOF analysis should be

independent of the applied bias voltage. A recent study using IFTOF

techniques has confirmed this fact [46]. There is nonetheless, an internal

field due to the space charge of the injected charge carrier packet. This

internal field is much smaller than the applied field, as the injected charge

is much smaller than CsV where Cs is the sample capacitance.

Figure 5.5 shows a typical IFTOF waveform with i(ti) and i(t2) clearly

discernible. IFTOF measurements were performed on a 195 p.m chlorine-

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doped a-Se:0.2%As film with an applied bias of 90 V for hole transport and

300 V for electron transport. The interruption time was varied and for each,

a measurement of i(ti) and i(t2) was made. The results of these

measurements are shown in the semi-logarithmic plots of Figures 5.6 and

5.7. The hole lifetime for this sample was found to be th=540.3 ;a and the

electron lifetime is '4=787.2 p.s. These lifetimes seem reasonable when

compared to the conventional TOF waveforms shown in Figure 5.1. The hole

TOF waveform show little or no decay since tT « Th. The electron TOF

waveform on the other hand exhibits an exponential decay. This is to be

expected as tT is of the same order as Te.

0 5 1/ 715 80

i(t2)

8 5 Time (m)

Figure 5.5 Typical IFTOF waveform for holes in a 195.1 p.m a-Se:0.2%As film showing i(ti), i(t2), and t1.

The exponential decay that the photocurrent undergoes, as shown in

Figures 5.6 and 5.7, is predicted by Equation 5.4 and more generally by

Equation 3.25 with 'CR-->00. The experimental verification of the exponential

decay of the photocurrent was described previously by Polischuk[47,48].

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This can be used as evidence that a single species (i.e. one with a single

trapping time) or set of traps, one for holes and another for electrons, is

responsible for deep trapping in a-Se alloys.

The product of the carrier mobility and the trapping lifetime wc is

known as the range of the carrier. The pr product is a measure of the

average drift length for a carrier per unit electric field before the carrier

becomes trapped. The range of the carriers is an important consideration for

the recombination experiment where the only decrease in free carrier

concentration should be due to recombination and not trapping. For the

samples used in the present study, the hole wc products are such that the

holes lost to trapping are insignificant when compared to the holes which

undergo recombination. However, the electrons have a more limited range

and electron trapping must be taken into account in the recombination

study.

5.4 Ambipolar Recombination Experiment

Processes such as electron-hole recombination play an important role

in the interpretation of the electronic properties of low mobility solids.

Experimental studies on orthorhombic sulphur crystals [36] and PVK:TNF

organic polymer films [49] have suggested that bulk recombination of

electrons and holes in low mobility solids is a diffusion controlled process

that agrees with Langevin's theory of recombination for gaseous ions [50,

51]. It has further been suggested that this diffusion controlled

recombination might be a universal property of low mobility solids.

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The theory proposed by Langevin was based on the assumption that

the mean free path of the carriers is small when compared to the

recombination radius rc. The latter is defined as the distance where the

potential energy due to Coulombic interactions between the hole and

electron is equal to kT where k is the Boltzmann constant and T is

temperature in degrees kelvin. rc is given by

e2

rc — 47ccoEykT

(5.5)

where Er is the relative dielectric constant of the medium. Assuming Er-6.6,

for a-Se rc-86A at room temperature. The mean free path of carriers, a, at

the mobility edge in a-Se has been estimated to be a.5-10A. It seems likely

that Langevin recombination behavior will be evident in a-Se since rc»a.

When an electron becomes trapped within a radius rc in the Coulomb

field of a hole, it will lose energy due to phonon interactions and

recombination will become highly probable. The recombination coefficient Cr

is directly proportional to the recombination cross-section ar and the relative

velocity of the electron and hole in the Coulomb field vr or Cr=0Arr. The

capture cross section, ar, is simply the surface area of a sphere with radius rc

surrounding the hole. The relative velocity, vr, can be found from the

relation

yr = Fc (14 +

where Fc is the Coulomb field. This leads to

83

(5.6)

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mobility. This leads to a photocurrent signal where the current due to the

hole packet "rides" on top of the electron current signal as in Figure 5.8(b).

Hole Injection time t= th

A

+ + ++ + + +

ip h

(a)

lectron Injection time t= to

x4

x=L

(b)

Figure 5.8 (a) Simplified schematic sketch of double injection TOF technique for studying recombination and (b) the resulting photocurrent.

85

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A typical photocurrent signal observed during the ambipolar TOF

recombination experiment is shown in Figure 5.9.

Hole Photocurrent

Phot

ocun

ent

(arb

. uni

t

Double Flash Photocurrent

6 Ti (el

100 200 300 400 Time (vs)

Figure 5.9 A typical photocurrent waveform from ambipolar TOF experiment. Insert shows an expanded view of the photocurrent due to the hole packet "riding" the top of the electron packet signal.

Consider Figure 5.10 where a hole charge packet drifts towards an

electron packet under the influence of an external field F. The two packets

meet each other at some time ti and have completely passed through each

other by time t2. Figure 5.10 illustrates the recombination events.

Considering hole drift with respect to the electron packet, at time ti, the hole

packet is at xi and recombination is just about to begin. At time t, the hole

packet is totally within the electron packet and the hole concentration is

decreasing due to recombination. Recombination stops when the hole packet

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exits the electron packet at X2 at time t2. If Sp and 8n are the changes in the

hole and electron concentrations due to recombination during a small

p

t+ St

LI)2 t2

1 i2

Figure 5.10 Schematic diagram of hole and electron packets passing through each other. It is assumed that n(x,t)»p(x,t).

interval of time St while the packets are interacting At=t2-t1, then the rate of

recombination is,

Sp Sn St = =—Cr n1).

(5.9)

Since Equation 5.9 is symmetrical in both p and n, the concentration

changes from ti to t2 follow

pi I)

87

(5.10a)

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or

78n j— = - Cr SP6t'

P2 In— = 1)1

1n = ni

(5.10b)

(5.11a)

(5.11b)

where p and if are some mean value of p and n in At. If p«n at all times so

that 71«n, then Equation 5.11 implies that n2-ni (i.e. there is no significant

change in n) and that the recombination primarily affects p. This is

attainable by maintaining the hole and electron photocurrent approximately

equal since 1.1.«µh which means n»p. Using Equation 5.11a, II can be

substituted for as follows. We can define the width of the electron packet as

AX=X2-X1 and therefore ii-a./(eAx). where ae is the injected negative charge

per unit area. At is related to Ax through the relative velocity of the electron

and hole charge packets where At=Ax/[(.thilte)F]. Substituting for n and At

in Equation 5.11a leads to

In P2 — CrogeP1 'e(Ete )F •

(5.12)

Both F and ae are experimentally determined parameters inasmuch

as F=Vo/L and ae is obtained by integrating the electron photocurrent in the

absence of hole injection and dividing the integral by the electrode area.

During the transit of the electrons across the sample, a small fraction of the

88

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electrons may be lost to deep traps within the mobility gap of the material.

This can be accounted for if the electron deep trapping lifetime tie is known

from the IFTOF analysis in the previous section. If Q. is the integrated

electron photocurrent without hole injection then

— exp(— t

+ t2 )

Q. 2t. A t T

exp(---t) (5.13)

where A is the electrode area. There is an upper and lower limit to ae. The

lower limit is due to the n»p requirement. The upper limit is the small

signal TOF requirement so that the internal field F is not space charge

perturbed. Since F remains constant throughout the experiment, the hole

and electron drift velocities remain constant and Equation 5.12 may be

rewritten as

In 'h2 CA

e(11. I-10F (5.14)

If the recombination coefficient is the Langevin coefficient, given by

Equation 5.8, then a substitution into Equation 5.14 will cause the

mobilities to be canceled and simply gives

i h2 In — 1h1

I a. cot, F

(5.15)

and a plot of ln(ihilim) versus ae/F should be a straight line whose slope is

simply -1/(eoer). Thus the fractional change in the hole photocurrent due to

89

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recombination is independent of the relative drift mobility of holes and

electrons. This is due to the fact that while the Langevin recombination

coefficient is directly pr'oportional to the relative mobility gr.(gh+ge), the

time duration of the overlap of the electron and hole packets is inversely

proportional to gr.

Figure 5.11 shows a semilogarithmic plot of the experimental ih2/ihi

values versus oe./F where ae, the injected negative charge, and F, the applied

electric field, are user defined experimental parameters. As shown in Figure

5.11, the experimental recombination data confirms the expected Langevin

recombination behaviour as predicted by Equation 5.15. The slope of the

line gives a value of er=6.35. This is very close to the value of er-.6.6 found

from capacitance measurements. This line was fit using the method of least

squares. The correlation coefficient, r, for this line was calculated to be

r=0.94. This verifies statistically the goodness of fit of the regression line.

It is also apparent that there is some scatter in the data but that over

a wide range of ae/F values, the best fit confirms Equation 5.15.

Experimental scatter is due to cre which involves integrating the electron

TOF photocurrent signal in the absence of injected holes. Variations in the

xenon flash output (about 5-15%) cause cre to be scattered by about this

amount. In addition, there are the usual experimental errors in the

measurement of ihdihi and the sample thickness L.

90

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0.0

-0.1

-0.2

-0.3

-0.4

-0.5

-0.6 00

• Sample 1 (1...1771.un)

ASample 2 (L=1951.tm)

0.5 1.0 1.5 2.0 2.5

CL/F (x10-11Cm'IV -I)

3.0 35

Figure 5.11 Semilogarithmic plot for ih2/ihi versus ae/F for two different stabilized a-Se samples. The slope of the line gives a relative dielectric constant of er=6.35. Correlation coefficient r=0.94.

5.5 Summary

Charge transport, charge trapping, and electron-hole recombination

were examined in chlorinated a-Se:0.2%As electroradiographic films. TOF

measurements were used to study charge carrier mobility. The hole mobility

was found to be 111=0.125 cm2V-1s-1 and the electron mobility was µe=0.0034

cm2v-i s Both hole and electron mobilities were relatively independent of

the applied field.

Deep trapping was investigated by using the IFTOF technique. The

exponential decay of the recovered photocurrent as a function of the

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interruption time suggests that deep trapping in a-Se is due to a single

species of localized traps within the mobility gap. Combining the results of

the TOF and IFTOF measurements yielded the p:r product or range of the

carriers. This property of the material determines how far a carrier will

travel before being trapped as a function of the applied field. The hole range

was wrh=67,54x10-6 cm2V-1, and the electron range was j.tte=2.68x10-6 cm2V-1.

For the samples being studied, the range of the electrons was such that the

electron trapping effect had to be taken into account during the

recombination experiment.

A double flash ambipolar TOF technique was used to study electron-

hole recombination. The results of the study were in agreement with those

predicted by the Langevin recombination theory. The predicted Langevin

recombination coefficient was Cer=35.2x10-9 cm3s-1. The experimentally

determined Langevin recombination coefficient was CrE=36.6x10-9 cm3s-1.

This result implies that the mean free paths of the carriers are very short

compared to the critical recombination radius. This type of recombination

could be a general property for those materials in which the mean free path

is much shorter than rc.

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6 CONCLUSIONS

Three different variations of the transient photoconductivity

measurement were used in completing this work. These were the

conventional time-of-flight (TOF), the interrupted field time-of-flight

(IFTOF), and the double flash, ambipolar time-of-flight techniques. These

techniques were applied to chlorinated a-Se:0.2%As electroradiographic

films to study charge carrier transport and recombination. The TOF and

IFTOF experiments were used to study charge carrier drift mobility and

deep trapping lifetime. The ambipolar TOF experiment was used to

examine charge carrier recombination. The combined results from these

three experiments can be used to provide an overall picture of charge carrier

transport in applications, such as electroradiography, where both electrons

and holes are involved.

Considerable effort was put into the design of the ambipolar TOF

experimental apparatus and into the development of a method to analyze

the results from this experiment. The essence of the ambipolar TOF

measurement involved photoinjecting oppositely charged carriers on

opposite sides of a sample. The two injected charge packets drifted towards

each other under the influence of an applied electric field. As the two

packets passed through each Other, some of the carriers underwent

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recombination. This recombination was evidenced by a fractional change in

the hole photocurrent.

The stabilized a-Se films were initially studied using the conventional

TOF method. These measurements provided a measure of the carrier drift

mobility as well as an indication of the amount of deep trapping expected.

The hole drift mobility, in the samples studied, was found to be

approximately 35 times larger than the electron mobility in the same

samples. The field dependence of the drift mobilities was also examined.

The hole mobility appears to have no field dependence at room temperature.

The electron drift mobility, on the other hand, shows a very slight field

dependence of the type geocF°•04. The origin of this field dependence is as yet

unknown but it is small enough that for a limited range of fields the electron

drift mobility can be assumed to be field independent.

The shape of the I-mode TOF waveforms can be used as a rough

indication of the amount of carrier deep trapping. There was no observable

decay in the hole photocurrent signal. This fact can be used to say that the

hole deep trapping lifetime, th, must be much greater than the hole transit

time, trh. However, the electron photocurrent signal did exhibit a decay.

This means that the electron deep trapping lifetime, tie, must be of the same

order as the electron transit time, tTe.

IFTOF analysis was then used to provide a measurement of the

charge carrier deep trapping lifetimes. The results confirmed that the hole

and electron deep trapping follow an exponential behaviour with a

characteristic trapping time, T. This exponential trapping behaviour implies

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a single species or set of traps are responsible for carrier deep trapping in

stabilized a-Se. Furthermore, the results confirmed the expectations that

t n,»Th and that t re was of the same order as t e.

The product of the carrier drift mobility, deep trapping lifetime, and

applied field, or wrF, called the Schubweg, provides a measure of the average

drift length for a charge carrier in a material. If this product is greater than

the thickness of the film being used, most carriers will travel across the film

without becoming trapped. In the present study, this was true for holes but

not for electrons. As a result, it became necessary to account for electron

deep trapping when performing the ambipolar recombination experiment.

It was demonstrated that the ambipolar TOF technique implemented

can be used to measure carrier recombination in stabilized a-Se films. An

electron packet of known charge•density per unit area, ige, was injected into

one side of a sample and a hole charge packet was injected into the opposite

side. The two packets drifted towards each other under the influence of an

applied electric field, F. The magnitude of the hole photocurrent was

measured before, ihi, and after, ih2, the packets had passed through one

another. The measured fractional change in hole photocurrent, ih2/ihi, as a

function of ae/F indicated that recombination in chlorinated a-Se:0.2%As

followed a Langevin type behaviour, as defined by the Langevin

recombination coefficient. This result directly implies that the carrier mean

free path, a, in stabilized a-Se, is much less than the critical recombination

radius rc. It is quite probable that this type of recombination is a general

property for materials that meet the a«re criterion, i.e., low mobility

materials. It seems that Langevin's simple formulation for recombination

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applies to amorphous semiconductors for which, at present, the rigorous

theoretical models are very limited.

Most current photoinduced discharge theories ignore charge carrier

recombination in their formulation. The importance of this work is that the

experimentally determined recombination coefficient can now be used in the

modeling of photoinduced discharge of stabilized a-Se photoreceptors used in

electroradiography, where both electron and hole drifts are involved in the

discharge process.

The combined use of different transient photoconductivity techniques

provides a powerful tool for studying charge transport and recombination in

high resistivity solids. Up to this point, this combination of measurements

has been applied only to stabilized amorphous selenium films. It would be

interesting to perform the same set of experiments on other low mobility

solids, in an effort to confirm the postulate that Langevin type

recombination is a general property for low-mobility materials. The current

experimental systems may have to be modified to incorporate different light

sources that correspond to the mobility gap of the new materials being

studied. It is also possible that the detection electronics may have to be

modified.

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