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Single Photon Detectors

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Single Photon Detectors By: Kobi Cohen Quantum Optics Seminar 25/11/09 Outline A brief review of semiconductors P-type, N-type Excitations Photodiode Avalanche ... – PowerPoint PPT presentation

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Title: Single Photon Detectors


1
Single Photon Detectors
  • By Kobi Cohen
  • Quantum Optics Seminar
  • 25/11/09

2
Outline
  • A brief review of semiconductors
  • P-type, N-type
  • Excitations
  • Photodiode
  • Avalanche photodiode
  • Geiger Mode
  • Silicon Photomultipliers (SiPM)
  • Photomultiplier
  • Superconducting Wire
  • Characterization of single photon sources
  • HBT Experiment
  • Second order correlation function

3
Semiconductors
4
Semiconductors
  • electrons and holes negative and positive
    charge carries
  • Energy-momentum relation of free particles, with
    different effective mass

5
Semiconductors
  • Thermal excitations make the electrons jump to
    higher energy levels, according to Fermi-Dirac
    distribution

6
Semiconductors
  • Excitations can also occur by the absorption of a
    photon, which makes semiconductors suitable for
    light detection

(T300K) Egap(eV) ?gap(nm)
Ge 0.66 1880
Si 1.11 1150
GaAs 1.42 870
7
Intrinsic Semiconductors
  • Charge carriers concentration in a semiconductor
    without impurities

8
N-type Semiconductor
  • Some impurity atoms (donors) with more valence
    electrons are introduced into the crystal

9
P-type Semiconductor
  • Some impurity atoms (acceptors) with less valence
    electrons are introduced into the crystal

10
The P-N Junction
  • Electrons and holes diffuse to area of lower
    concentration
  • Electric field is built up in the depletion layer
  • Drift of minority carriers
  • Capacitance

11
Biased P-N junction
  • When connected to a voltage source, the i-V curve
    of a P-N junction is given by
  • Well focus on reverse biasing
  • larger electric field in the junction
  • extended space charge region

12
The P-N photodiode
  • Electrons and holes generated in the depletion
    area due to photon absorption are drifted
    outwards by the electric field

13
The P-N photodiode
  • The i-V curve in the reverse-biased P-N junction
    is changed by the photocurrent
  • Reverse biasing
  • Electric field in the junction increases quantum
    efficiency
  • Larger depletion layer
  • Better signal

14
The P-I-N junction
  • Larger depletion layer allows improved efficiency
  • Smaller junction capacitance means fast response

15
Detectors Quantum Efficiency
  • The probability that a single photon incident on
    the detector generates a signal
  • Losses
  • reflection
  • nature of absorption
  • a fraction of the electron hole pairs recombine
    in the junction

16
Detectors Quantum Efficiency
  • Wavelength dependence of a

17
Summary P-N photodiode
  • Simple and cheap solid state device
  • No internal gain, linear response
  • Noise (dark current) is at the level of several
    hundred electrons, and consequently the smallest
    detectable light needs to consist of even more
    photons

18
Avalanche photodiode
  • High reverse-bias voltage enhances the field in
    the depletion layer
  • Electrons and holes excited by the photons are
    accelerated in the strong field generated by the
    reverse bias.
  • Collisions causing impact-ionization of more
    electron-hole pairs, thus contributing to the
    gain of the junction.

19
Avalanche photodiode
P-N photodiode
Avalanche photodiode
20
Summary APD
  • High reverse-bias voltage, but below the
    breakdown voltage.
  • High gain (100), weak signal detection (20
    photons)
  • Average photocurrent is proportional to the
    incident photon flux (linear mode)

21
Geiger mode
  • In the Geiger mode, the APD is biased above its
    breakdown voltage for operation in very high
    gain.
  • Electrons and holes multiply by impact ionization
    faster than they can be collected, resulting in
    an exponential growth in the current
  • Individual photon counting

22
Geiger mode quenching
  • Shutting off an avalanche current is called
    quenching
  • Passive quenching (slower, 10ns dead time)
  • Active quenching (faster)

23
Summary Geiger mode
  • High detection efficiency (80).
  • Dark counts rate (at room temperature) below
    1000/sec. Cooling reduces it exponentially.
  • After-pulsing caused by carrier trapping and
    delayed release.
  • Correction factor for intensity (due to dead
    time).

24
Silicon Photomultipliers
  • SiPM is an array of microcell avalanche
    photodiodes (20um) operating in Geiger mode,
    made on a silicon substrate, with 500-5000
    pixels/mm2. Total area 1x1mm2.
  • The independently operating pixels are connected
    to the same readout line

25
SiPM Examples
26
Summary SiPM
  • Very high gain (106)
  • Dark counts 1MHz/mm2 (20C) to 200Hz/mm2 (100K)
  • Correction factor (other than G-APD)

27
Photomultiplier
  • Photoelectric effect causes photoelectron
    emission (external photoelectric effect)

For metals the work function W 2eV, useful for
detection in the visible and UV. For
semiconductors can be 1eV, useful for IR
detection
28
Photomultiplier
  • Light excites the electrons in the photocathode
    so that photoelectrons are emitted into the
    vacuum
  • Photoelectrons are accelerated due to between the
    dynodes, causing secondary emission

29
Summary Photomultiplier
  • First to be invented (1936)
  • Single photon detection
  • Sensitive to magnetic fields
  • Expensive and complicated structure

30
A remark image intensifiers
  • A microchannel plate is an array consists of
    millions of capillaries (10 um diameter) in a
    glass plate (1mm thickness).
  • Both faces of the plate are coated by thin metal,
    and act as electrodes.
  • The inner side of each tube is coated with
    electron-emissive material.

31
Superconducting nano-wire
  • Ultra thin, very narrow NbN strip, kept at 4.2K
    and current-biased close to the critical current.
  • A photon-induced hotspot leads to the formation
    of a resistive barrier across the sensor, and
    results in a measurable voltage pulse.
  • Healing time 30ps

32
SSPD meander configuration
  • Meander structure increases the active area and
    thus the quantum efficiency

33
  • End of 1st part !

34
Hanbury Brown-Twiss Experiment (1)
  • Back in the 1950s, two astronomers wanted to
    measure the diameters of stars

35
Hanbury Brown-Twiss Experiment (2)
36
Hanbury Brown-Twiss Experiment (3)
  • In their original experiments, HBT set t0 and
    varied d.
  • As d increased, the spatial coherence of the
    light on the two detectors decreased, and
    eventually vanished for large values of d.

37
Coherence time
  • The coherence time tc is originated from atomic
    processes
  • Intensity fluctuations of a beam of light are
    related to its coherence

38
Correlations (1)
  • We shall assume from now on that we are testing
    the spatially-coherent light from a small area of
    the source.
  • The second order correlation function of the
    light is defined by

(Why second order?)
39
Correlations (2)
  • For t much greater than the coherence time

40
Correlations (3)
  • On the other and, for t much smaller than the
    coherence time, there will be correlations
    between the fluctuations at the two times. In
    particular, if t0

41
Correlations example
  • If the spectral line is Doppler broadened with a
    Gaussian lineshape, the second order correlation
    functions is given by

42
Summary correlations in classical light
43
HBT experiments with photons
  • The number of counts registered on a photon
    counting detector is proportional to the intensity

44
Photon bunching and antibunching
  • Perfectly coherent light has Poissonian photon
    statistics
  • Bunched light consists of photons clumped together

45
Photon bunching and antibunching
  • In antibunched light, photons come out with
    regular gaps between them

46
Experimental demonstration of photon antibunching
  • Antibunching effects are only observed if we look
    at light from a single atom

47
Experimental demonstration of photon antibunching
  • Antibunching has been observed from many other
    types of light emitters

48
Bibliography
  • Fundamentals of Photonics, Saleh Teich, Wiley
    1991
  • Quantum Optics An introduction, Mark Fox, Oxford
    University Press 2006
  • Hamamatsu MMPC datasheet (online)
  • PerkinElmer APCM datasheet (online)
  • Goltsman G., SSPD, APL 79(6),2001, 705-707
  • Hanbury Brown, R. , and Twiss, R. Q. , Nature,
    177, 27 (1956)
  • Hanbury Brown, R. , and Twiss, R. Q. , Nature,
    178, 1046 (1956)
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