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1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 1: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 2: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 3: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 4: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 5: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 6: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 7: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Page 8: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

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Performance of the RICH detectors of LHCb

Antonis PapanestisSTFC - RAL

for the LHCb Collaboration

Page 9: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Outline

Detector description: See previous talk by Davide

Perego.

Cherenkov angle resolution Alignment Corrections for the

magnetic field distortions. Particle identification

PID algorithm. Small selection of physics

results that depend on particle ID.

9

Monte Carlo simulation of the invariant mass for B->hh decays

Page 10: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Cherenkov angle resolution (i)

10

Typical run

σ= 1.62 mrad σ= 0.68 mrad

Page 11: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Cherenkov angle resolution (ii)

11

Resolution distribution of all 2010 runsVery good stability in time

1.63 mrad

0.68 mrad

Resolution in time

RICH1

RICH2

Page 12: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Using isolated rings

12

Cherenkov angle vs momentum in RICH1

Page 13: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

PID algorithm

Global event likelihood algorithm. Likelihood function includes

expected contributions from signal plus background for every pixel.

Signal photons come from the track that generated the ring, background can be noise or Cherenkov light from other tracks.

The whole event is considered as a whole.

Performs better than methods that treat every track separately, especially at high occupancies with overlapping rings.

13

Page 14: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Pure particle samples

14

†Nucl. Inst. & Meth. A 555 (2005) 356-369

σ=3.0 MeVσ=1.5 MeV

σ=1.0 MeV

Page 15: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

PID performance

15

Improvement expected at the next reprocessing

K/ p/

Page 16: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

RICH physics potential

16

Page 17: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Physics analysis (i)

17

Measurement of direct CP violation in charmless charged two-body B decays at LHCb (LHCb-CONF-2011-011)

KB

B KKB

Without PID dominated by:

with kinematic cuts onlyhhB

Page 18: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Physics Analysis (ii)

18

Measurement of the relative yields of the decay modes B0→D−π+ ,B0 → D−K+ , B0s → D−

s π + , and determination of fs/fd for 7 TeV pp collisions (LHCb-CONF-2011-013)

DBd DKBd

No combinatorial background

Page 19: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Philips Digital Photon Counting(PDPC)Dr. York HämischSenior DirectorPhilips Corporate Technologies

SiPM’s: from analog to digital, from laboratory to application

Page 20: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

20

Digital Silicon Photomultipliers (dSiPM) -The next solid state (digital) revolution?

Transistor Television

X-Ray imaging

Digital Camera

Digital Photon Counting

Page 21: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

21

PDPC: short history

2004 Research project: “Novel technologies for future PET systems”

2005 Dr.Thomas Frach invented the digital SiPM

2006 Research project: “Integrated digital light sensor”; first test chip with promising results (inkubator)

2006 Disentanglement of Philips Semiconductors – now NXP

2007 Start of the PDPC venture

2008 Proof of concept

2009 Technology launch at IEEE NSS-MIC sensor V1.0

2010 PDPC separate unit of Philips Corporate Technologies

2011 Introduction of PDPC-TEK (Technology Evaluation Kit) and sensor version 2.0

Page 22: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Initial Motivation: A better detector for Positron- Emission-Tomography (PET) with TOF and DOI

Graphics courtesy of Spanoudaki & Levin, Stanford,in: Phys. Med. Biol. (56) 2011

TOF – time-of-flight

DOI – depth of interaction

Page 23: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

23

From single APD to multiple SPAD’s:Single Geiger-mode APD

Geiger-mode APD Array (SPAD’s):“Silicon Photomultiplier”

B. Dolgoshein, V. Saveliev, V. GolovineFirst idea: Russia, early 80‘s

• fully analog• poor timing• high bias voltage, but

below breakdown

• single photon resolution• binary, but still analog• better timing• low bias voltage, above breakdown

Page 24: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

(S)APD in Geiger-ModeE

xt.

Vo

ltag

eC

urr

ent

Time

VBD

Meta-stable

Breakdown

Quenching

Page 25: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

25

SiPM-SPAD’s: sensitivity vs. dynamic range

Photographs courtesy of Spanoudaki & Levin, StanfordSensors, 10, 2010

Page 26: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital Photon Counting: the concept

Intrinsically, the SiPM is a digital device:

A single cell (SPAD) breaks down or not.

It works like a switch:

no breakdown: „0“ – no photonbreakdown: „1“ – single photon

Therefore, while the APD is a linear amplifier for the input optical signal with limited gain, the SPAD is a trigger device so the gain concept is meaningless.(source: Wikipedia)

Page 27: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital Photon Counting: realization

analog SiPM

www.hamamatsu.com

Summing all cell outputs leads to an analog output signal and limited performance

TDC andphoton counter

Digital output of• Number of photons• Time-stamp

Digital Cells

digital SiPM (dSiPM)

Integrated readout electronics is the key element to superior detector performance

Page 28: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Analog vs. Digital SiPM

28

Page 29: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: Principle

Page 30: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: Principle

Page 31: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: Principle

Page 32: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: Principle

Page 33: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: architecture and pixel diagram

33

Single pixel

Die (2 x 2pixel)

(smart) tile (8x8 pixel)

Page 34: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM array (tile 2.0)advanced integration

34

FPGA/Flash:

• tile firmware• data collection/concentration• Skew correction• Saturation correction• configuration• temperature measurement • dark count maps

200 MHz ref. clock

Power (1.2V, 1.8V, 2.5V, 3.3V, 30V)

SPI interface

Serial Dataoutput(x2)

Page 35: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

Digital SiPM: Typical acquisition sequence (example)

Page 36: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

PDPC dSiPM: intrinsic timing resolution

PDPC array

USB

Coincidencedetection

PDPC array

Clock,Config,Data

Clock,Config,

Data

PCFPGA board FPGA board

electronic trigger

36

psec-laser

-100 -80 -60 -40 -20 0 20 40 60 80 1000

10000

20000

30000

40000

50000

60000

70000

Co

un

ts (

arb

. u

.)

Timestamp difference (ps)

(44 ± 1) ps FWHM

-120 -80 -40 0 40 80 1200

10000

20000

30000

Co

un

ts

Timestamp difference (ps)

Timing jitter: 44 ps FWHM 59 ps FWHM

Page 37: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

PDPC: scintillator coincidence setup

37

Recently achieved 120 ps FWHM using LSO:Ca

(Schaart et.al., TU Delft,submitted to IEEE-MIC)

Page 38: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

PDPC dSiPM: Dark count mapWorst cells are switched off

• Dark counts per second at 20°C and 3.3V excess voltage

• ~ 95% good diodes (dark count rate close to average)

• Typical dark count rate at 20°C and 3.3V excess voltage: ~150Hz / diode

• Dark count rate drops to ~1-2Hz per diode at -40°C

Page 39: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

PDPC dSiPM: slow scan imaging mode

Page 40: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

PDPC dSiPM: crosstalk reduction by trenches

Page 41: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

41

Comparison of light detectors – which one is going to win?

Table courtesy of Spanoudaki & Levin, Stanfordin: Sensors, 10, 2010

PDPCdSiPM

meaninglessfirst photon

25-75< 350.33No

mm²-m²Currently: ~25

Page 42: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

A digital light sensor might beuseful beyond PET

?

?

ClinicalPET

imaging

Pre-clinical

PET&SPECT

PET/MR

ClinicalSPECTimaging

SpectralCT

Focus Nuclear Imaging

Adjacent opportunities

Low dose CT

Other Medical Imaging Analytical Instrumentation

High Energy Physics

Night Vision / Surveillance / Security

DNA Sequencing

Microscopy

Microarrays

Antineutrino Detection

Particle Accelerators

Automotive Night Vision

LIDAR

Facility/Homeland

Security

Cherenkov Detectors

?

LoC

Medical Imaging

Intra-operativeprobes

Page 43: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

4343

Key parameters of light detectors

λ

sens.

res.

speed

timingdyn. range

size

priceKey parameters:

1. Wavelength2. Sensitivity3. Spatial resolution4. Speed5. Timing6. Dynamic range7. Size8. Price

Page 44: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

4444

What does the ideal spider web for HEP look like?

Key parameters:

1. Wavelength2. Sensitivity3. Spatial resolution4. Speed5. Timing6. Dynamic range7. Size8. Price

λ

sens.

res.

speed

timingdyn. range

size

price

Page 45: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

YH ©Philips Digital Photon Counting, February 2011

Philips Digital Photon Counting

www.philips.com/digitalphotoncounting

[email protected]

Thank you for your attention!

Page 46: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

•Makoto Tabata•Japan Aerospace Exploration Agency (JAXA)•TIPP 2011 in Chicago

Recent Progress in Silica Aerogel Cherenkov Radiator

Page 47: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Makoto TabataJapan Aerospace Exploration Agency (JAXA)

TIPP 2011 in Chicago

Recent Progress in Silica Aerogel Cherenkov

Radiator

Page 48: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Silica Aerogel

1

Silica aerogel is a 3D structural solid of SiO2 particles.

Scanning electron microscope image 10 mg/cc silica aerogel (magnification: x 100,000)

• porous (>99% air)low bulk densitythermal insulator

• transparentΟ(10) nm SiO2 particlesRayleigh scattering

• feel like styrofoam

30 mg/ccsilica aerogel

100 nm

Page 49: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

1st method: Single-step method2nd method: Two-step method world standard3rd method: KEK method our original

1.Wet-gel synthesis (sol-gel step) We have various preparation recipes for chemicals.

2.Aging3.Hydrophobic treatment our original4.CO2 supercritical drying 1 month in total

Conventional Production Method

3

CO2 autoclave

extract liquid component of wet-

gel through supercritical drying

Wet-gel

Hydrophobic

Refractive index (density) can be controlled in the sol-gel step.

Page 50: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

1.Wet-gel synthesis (1st density control)2.Aging3.Pin-drying (2nd density control)

4.Hydrophobic treatment5.CO2 supercritical drying

Pin-drying Production Method

7

1.00

1.05

1.10

1.15

1.20

1.25

1.30

0.5 0.6 0.7 0.8 0.9 1.0

length contraction

refr

activ

e in

dex

n0 = 1.06

shrink

original non-shrink aerogel

Semi-sealed container with some pin-holes

several weeks

Pin-drying (PD) method is 4th method to produce aerogelwith high refractive index. need additional time

for the pin-drying process

methanol solvent

Partial evaporation of solventpin-

hole

Page 51: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

Reproducibility in PD Method

8

1.10

1.15

1.20

1.25

1.30

20% 30% 40% 50%

wet-gel weight

refr

activ

e in

dex

Target n = 1.25 (20 tiles)Target n = 1.20 (10 tiles)

Target n = 1.12 (10 tiles)0.01

0.01

0.005

Target refractive index is well-controlledby monitoring wet-gel weight.

40 tiles were produced forn = 1.25, 1.20 and 1.12.

(Wet-gels were synthesizedfor n0 = 1.06 usingmethanol solvent.)

Refractive index fluctuations were evaluated at each

target index.

Page 52: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

0

10

20

30

40

50

60

70

1.00 1.05 1.10 1.15 1.20 1.25 1.30

refractive index

tran

smis

sion

leng

th [m

m]

Conventional (Ethanol)

Conventional (Methanol)

Conventional (DMF)

PD (Methanol)

Expansion of High Index Range in 2005

10

Original (non-shrink) aerogeln = 1.06 (methanol)

Ultra-high refractive index (n > 1.10) aerogels with sufficienttransparency (Λ > 20 mm) were developed.

Entirely newrefractive index range

Methanol solvent

Page 53: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

0

10

20

30

40

50

60

70

1.00 1.05 1.10 1.15 1.20 1.25 1.30

refractive index

tran

smis

sion

leng

th [m

m]

Conventional (Ethanol)Conventional (Methanol)Conventional (DMF)PD (Methanol)PD (DMF)

Improvement of Transparency in 2008

11

Original (non-shrink) aerogeln = 1.066 (DMF)

The transmission length was improved in n > 1.10.

It takes long pin-drying process because DMF is difficult to evaporate.

DMF solvent

Page 54: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

0

10

20

30

40

50

60

70

1.00 1.05 1.10 1.15 1.20 1.25 1.30

refractive index

tran

smis

sion

leng

th [m

m]

Conventional (Ethanol)Conventional (Methanol)Conventional (DMF)PD (Methanol)PD (DMF)

The Most Transparent Sample in 2008

12

Original (non-shrink) aerogeln = 1.049 (DMF)

The highest transparency (Λ > 50 mm) was obtained in n ~ 1.06.

DMF solvent

1.003 < n < 1.26 available

Page 55: 1. 2 3 4 5 6 7 8 Performance of the RICH detectors of LHCb Antonis Papanestis STFC - RAL for the LHCb Collaboration

• n = 1.05 + 1.06, 2 cm thick each (total 4 cm thick)

Np.e. = 10.6 (conventional) 13.6 (improved)60% ring acceptance

• 1.10 < n < 1.231 cm thick each Np.e. = 5-10 (new data)50% ring acceptance

Photoelectron Yield

14

0

2

4

6

8

10

12

1.00 1.05 1.10 1.15 1.20 1.25refractive index

Np.

e./t

rack

MethanolDMFClear Cherenkov

rings were observed.

Standard method

PD method

TransparencyDMF > Methanol

Sufficient photoelectrons were detected.

1 cm thick