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Light Engineering in New Materials How material science can help in realizing new efficient incoherent and coherent light sources April 15, 2019 Lights of Tuscany 2019 Anna Vinattieri, Dept. Physics and Astronomy, UNIFI 1

Light Engineering in New Materialsai-sf.it/lot19/files/Slides/vinattieri.pdf · 2019. 11. 27. · Light Engineering in New Materials How material science can help in realizing new

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  • Light Engineering in

    New MaterialsHow material science can help in realizing new

    efficient incoherent and coherent light sources

    April 15, 2019Lights of Tuscany 2019

    Anna Vinattieri, Dept. Physics and Astronomy, UNIFI

    1

  • Outline

    A little bit of history

    Band-gap engineering

    Epitaxial growth

    Chemical synthesis

    Perovskites

    A look to the future

    April 15, 2019Lights of Tuscany 2019 2

  • A little bit of history: 150 years from the

    Mendeleev Table

    April 15, 2019Lights of Tuscany 2019

    The semiconductor tree

    The Mendeleev table is the tree

    principal root

    3

  • The recognition of material science

    relevance

    April 15, 2019Lights of Tuscany 2019 4

    The nanostructures and

    the superconductors

  • April 15, 2019Lights of Tuscany 2019 5

    Heterostructures

    and integrated

    circuit

  • April 15, 2019Lights of Tuscany 2019

    The CCD

    6

  • April 15, 2019Lights of Tuscany 2019

    7

    The Graphene: the

    perfect lattice

  • April 15, 2019Lights of Tuscany 2019

    8

    The

    blue/white

    laser diodes

  • The materials for opto-devices

    April 15, 2019Lights of Tuscany 2019

    SemiconductorsSemiconductors

    Ordered structures ( bulk crystals and nanostructures)

    Ordered structures ( bulk crystals and nanostructures)

    InorganicInorganic

    OrganicOrganic

    AmorphousAmorphous

    9

  • The Rosetta Stone of Semiconductors

    April 15, 2019Lights of Tuscany 2019 10

  • The King of Semiconductors for

    electronics: Silicon

    April 15, 2019Lights of Tuscany 2019

    32 inch , 80 cm

    Unfortunately Si is very bad for

    light emitters being an indirect

    band-gap semiconductor, so it is

    hard to have electrons and holes

    recombining in a radiative way !

    11

  • The Kings of Semiconductors for light

    emitters : III-V and III-Nitrides

    In,Ga,Al Arsenide and Nitride Alloys with a band gap value

    ranging from 0.8 to 4 eV

    We can realize a device emitting light from 1.55 µm ( perfect

    for telecomm) and 300 nm ( perfect for UV- lithography and

    blue-rays, UV curing, etc.). White LEDs are realized using

    nitride alloys.

    April 15, 2019Lights of Tuscany 2019

    colours.

    12

  • How materials are realized?

    April 15, 2019Lights of Tuscany 2019

    Czochralski growth (1916): very fast for big

    crystals : O and C common contaminants

    Epitaxial growth developed in late 1960s in

    Bell Labs

    AA 2018/19

    growth speed

    ~ 2 - 3

    mm/minute

    Fisica dei Semiconduttori:Teoria e Applicazioni 13

  • Molecular Beam Epitaxy

    April 15, 2019Lights of Tuscany 2019 14

  • Epitaxy can be by Molecular Beam,

    Chemical Vapour, Liquid Phase

    April 15, 2019Lights of Tuscany 2019

    Epitaxy means in “ growth in an ordered way”: epitaxial growth is

    therefore a growth with an high control of the deposition, at the atomic

    level

    It requires same

    crystallographic

    lattice and

    “same” lattice

    constant to avoid

    extended defects

    which are

    detrimental for

    the device

    operation

    15

  • But Nature can help: Self-assembled growth

    April 15, 2019Lights of Tuscany 2019 16

  • Some results

    April 15, 2019Lights of Tuscany 2019 17

    A superlattice

    Quantum dots

  • What’s the meaning?

    We can modify the electronic properties ( energy, band

    dispersion, band gap…) at the nanoscale ( few Angstrom up

    to tens of nm)

    Quantum effects dominate and we can tailor the

    material properties the way we prefer

    April 15, 2019Lights of Tuscany 2019 18

  • So very nice results but…..

    Highly expensive techniques

    April 15, 2019Lights of Tuscany 2019 19

    As alternative:

    Chemical synthesis

  • Advantages of chemical synthesis

    Low cost synthesis and processing

    High tunability of band-gap

    Easier integration in photonic structures

    April 15, 2019Lights of Tuscany 2019 20

  • The promising class of materials:

    Perovskites

    April 15, 2019Lights of Tuscany 2019 21

    Same class of material

    as CaTiO3

    A:Ca2+

    B:Ti4+

    X:O-

    Depending on A, they can be

    hybrid with organic cation or

    fully inorganic

    A: CH3NH3, Cs

    B:Pb,Sn

    X:Cl,Br,I

  • Application Fields

    April 15, 2019Lights of Tuscany 2019 22

    Energy Harvesting

  • LEDs and Lasers

    April 15, 2019Lights of Tuscany 2019 23

    https://doi.org/10.1016/j.mattod.2017.03.021

    https://doi.org/10.1016/j.mattod.2017.03.021

  • Different material nanostructuring

    means different behavior

    April 15, 2019Lights of Tuscany 2019 24

    From bulk to plates, wires, dots

  • Here in Florence

    April 15, 2019Lights of Tuscany 2019 25

    • Synthesis

    • Morphological and structural characterization (XRD, SEM)

    • High resolution optical spectroscopy in space and time

  • Synthesis of nanostructures/thin films

    April 15, 2019Lights of Tuscany 2019 26

  • Then precursors are spin-coated on a

    substrate……..solvent evaporation produces

    perovskite

    April 15, 2019Lights of Tuscany 2019 27

  • For crystals

    April 15, 2019Lights of Tuscany 2019 28

  • April 15, 2019Lights of Tuscany 2019 29

    At the optical microscope:

    spin-coated samples

  • High resolution Imaging

    SEM AFM

    April 15, 2019Lights of Tuscany 2019 30

  • April 15, 2019Lights of Tuscany 2019 31

    High resolution SEM

  • Bulk crystals

    April 15, 2019Lights of Tuscany 2019 32

    Using an optical microscope Using a SEM

  • What spectroscopy on such samples?

    April 15, 2019Lights of Tuscany 2019 33

    ➢We need to determine the bandgap: standard cw

    spectroscopy ( transmission/ absorption/ photoluminescence)

    ➢We need to understand the non-radiative recombination

    paths: temperature-dependent measurements

    ➢We need to understand the carrier interactions and the

    recombination kinetics: time-resolved experiments, typically

    at the picosecond time-scale

  • Moreover: optical spectroscopy at the

    macro or micro scale?

    April 15, 2019Lights of Tuscany 2019 34

    Macro: we probe macroscopic portions of the sample ( ≥ 100 µm2)

    Micro: Spatial resolution at the diffraction limit (≈µm in the vis)

    Near Field detection: spatial resolution limited by the fiber tip

    ( ≈ 100 nm)

    Different informations can be extracted!

  • Here in the labs

    April 15, 2019Lights of Tuscany 2019 35

  • MicroPL

    April 15, 2019Lights of Tuscany 2019 36

  • SNOM

    April 15, 2019Lights of Tuscany 2019 37

  • April 15, 2019Lights of Tuscany 2019 38

    At the end

  • Some examples

    Superlinear emission: ASE or lasing?

    April 15, 2019Lights of Tuscany 2019 39

    1.61 1.62 1.63 1.64 1.65

    1.61 1.62 1.63 1.64 1.65

    Energy (eV)

    P = I0

    P = 1.6 I0

    P = 2.3 I0

    PL

    Inte

    nsi

    ty (

    a.u.)

    P = 3.4 I0

    P = 5.4 I0

    1.60 1.61 1.62 1.63 1.64

    1.60 1.61 1.62 1.63 1.64

    Energy (eV)

    P= I0

    P=5 I0

    P=60 I0

    PL

    In

    ten

    sity

    (a.

    u.)

    P=85 I0

    P=140 I0

  • Decay kinetics is similar

    but polarization

    properties are different

    April 15, 2019Lights of Tuscany 2019 40

    0.0 0.2 0.4 0.6 0.8 1.010

    -2

    10-1

    1

    400ps

    400ps

    Experimental response

    SE

    SPE

    No

    rmal

    ized

    PL

    In

    ten

    sity

    Time (ns)

  • Surface states role

    April 15, 2019Lights of Tuscany 2019 41

    10-1

    1

    10-2

    10-1

    1

    Norm

    . P

    L I

    nte

    nsi

    ty

    293 K

    11 K

    P

    DCNorm

    . P

    L I

    nte

    nsi

    ty

    Time 1ns

    11K

    293K

    P

    BAA11 K

    210 K

    P

    A

    Time 1ns

    11K

    293KP

    2.3 2.4 2.5 2.60.0

    0.2

    0.4

    0.6

    0.8

    1.0

    Norm

    aliz

    ed P

    L I

    nte

    nsi

    ty

    C

    D

    B

    Energy (eV)

    A

    Recombination dynamics slows

    down increasing the

    temperature!

    The smaller the nanocrystals,

    the larger the effect

    0.00 0.02 0.04 0.06 0.08 0.10

    A

    Inte

    gra

    ted

    PL

    In

    ten

    sity

    1/Temperature (K-1)

    T = 10 K

    2.2 2.3 2.4 2.5 2.6 2.7

    293K

    130K

    230K

    210K

    180K

    150K

    110K

    90K

    70K

    50K

    30K

    11K

    250K

    PL

    In

    ten

    sity

    (a.

    u.)

    Energy (eV)

    ABC

    D

  • The increase of lifetime with T is counterintuitive ! Usually

    non radiative channels are more effective as T increases

    But….

    April 15, 2019Lights of Tuscany 2019 42

    Large crystals or high temperature (smaller barrier, less surface defects)

    Small crystals or low temperature (larger barrier, more surface defects)

    CB

    VB

    Surface state

    Surface states act as a

    reservoir an can release

    population as T increases

  • April 15, 2019Lights of Tuscany 2019 43

    Band A (K-1) B (10-3K-2) EB (meV)

    A

    ≈ 10-3

    0.18 33

    B 0.48 39

    C 2.6 67

    D 25 130

    Thermally activated transfer

    0 50 100 150 200 250 300

    1

    10

    P/P

    0

    Temperature (K)

    A

    B

    C

    D

    P0= P(T=10K)

    c

    𝑷 𝑻 = 𝑨𝑻 + 𝑩𝒆−𝑬𝑩𝒌𝑩𝑻

  • Non-linearities

    with two beams

    April 15, 2019Lights of Tuscany 2019 44

    nanop2018-R

    om

    e O

    cto

    ber

    1-3

    44

    Non resonant bias CW @ 405

    nm + ps pulse @ 370 nm

    Ipb- (Ip+Ib) vs time

  • Negative signal: bleaching related to

    localized/bound states

    Positive signal: Superlinearity from excitons

    formation

    April 15, 2019Lights of Tuscany 2019 45

    2.26 2.28 2.3 2.32 2.34 2.36

    0ps

    14.2ps

    28.4ps

    42.6ps

    I pb-(I p

    +I b

    )

    Energy(eV)

    0

    E0= zero crossing energy

    2.26 2.28 2.3 2.32 2.34 2.36

    56.8ps85.2ps113.6ps142ps184.6ps227.2ps269.8ps

    I pb-(I p

    +I b

    )

    Energy(eV)

    0

  • Conclusions

    Optical spectroscopy implemented in several different configurations allows to

    provide a dramatic amount of physical information which is fundamental for the

    progress of material science.

    New classes of artificial-made materials recently realized are of relevance for

    opto devices: in these years perovskites are probably the most investigated !

    April 15, 2019Lights of Tuscany 2019 46

  • A look to the future

    Controlled deposition of nanocrystals and homogeneous

    film

    Definition of post-growth treatment for defect annealing

    Coupling of perovskites to photonic structures to tailor the

    light properties

    Optimization of electrical injection for realization of Leds

    and Lasers

    Eco-friendly materials ( no lead, etc)

    April 15, 2019Lights of Tuscany 2019 47

  • Let’s try to think our lives without

    semiconductors: just 3 objects

    April 15, 2019Lights of Tuscany 2019 48

  • Could you survive?

    Thanks

    April 15, 2019Lights of Tuscany 2019 49