Photodetectors Read: Kasip, Chapter 5 Yariv, Chapter 11...

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Photodetectors Read: Kasip, Chapter 5 Yariv, Chapter 11 Class Handout ECE 162C Lecture #13 Prof. John Bowers

Transcript of Photodetectors Read: Kasip, Chapter 5 Yariv, Chapter 11...

  • Photodetectors Read: Kasip, Chapter 5

    Yariv, Chapter 11 Class Handout

    ECE 162C Lecture #13

    Prof. John Bowers

  • Definitions

    •  Quantum efficiency η: Ratio of the number of electrons collected to the number of photons incident.

    •  Responsivity: current out divided by optical power incident

    AWhc

    eheRd /24.1

    ηληλ

    νη ===

  • External Quantum Efficiency and Responsivity

    Different contributions to the photocurrent Iph. Photogeneration profiles corresponding to short, medium and long wavelengths are also shown.

    Schematic photogeneration profiles

  • photonsincident ofNumber collected and generated EHPfree ofNumber

    =eη

    External quantum efficiency (QE) ηe of the detector

    υη

    hPeI

    o

    phe /

    /=

  • Responsivity R

    o

    ph

    PI

    ==(W) Power OpticalIncident

    (A)nt PhotocurreR

    hce

    he

    eeλ

    ηυ

    η ==R

  • Responsivity R

    Responsivity (R) vs. wavelength (λ) for an ideal photodiode with QE = 100% (ηe = 1) and for a typical inexpensive commercial Si photodiode. The exact shape of the responsivity curve depends on the device structure.

    The line through the origin that is a tangent to the responsivity curve at X, identifies operation at λ1 with

    maximum QE

  • pin Photodiode

    The responsivity of Si, InGaAs and Ge pin type photodiodes. The pn junction GaP detector is used for UV detection. GaP (Thorlabs, FGAP71), Si(E), IR enhanced Si (Hamamatsu S11499), Si(C),

    conventional Si with UV enhancement, InGaAs (Hamamatsu, G8376), and Ge (Thorlabs, FDG03). The dashed lines represent the responsivity due to QE = 100 %, 75% and 50 %.

  • pin Photodiode

    WV

    WV rr

    o ≈+= EE

    WAC roεε=dep

    d

    Wtv

    =drift

  • pin Photodiode

    Drift velocity vs. electric field for holes and electrons in Si.

    d

    Wtv

    =drift

    Width of i-region (Depletion region)

    Drift velocity Transit time (Drift time)

  • pin Photodiode Speed

    A reverse biased pin photodiode is illuminated with a short wavelength light pulse that is absorbed very near the surface. The photogenerated electron has to diffuse to the depletion region where it is swept into the i-layer and drifted across.

    In time t, an electron, on average, diffuses a distance given by

    = (2Det)1/2

    Electron diffusion coefficient

  • PIN Impulse Response?

  • PIN Impulse Response?

    Levevj hhee σσ +=

    Displacement current flows. That is what is measured in an external circuit, not conduction current.

  • Avalanche Photodiodes (APDs) •  α Rate at which electrons multiply •  β Rate at which holes multiply

    •  A large ratio of α/β or β/α results in a large gain bandwidth product and low noise amplification. True for Si

    •  Most III-Vs have a small ratio, and limited gain bandwidth product. The noise is larger, but still lower than a PIN receiver.

  • E l e c t r i c F i e l d [ k V / c m ]

    I n 0 . 5 3 G a 0 . 4 7 A s e l e c t r o n s h o l e s

    G a A s e l e c t r o n s h o l e s

    I n P h o l e s

    e l e c t r o n s

    F r o m : S i : P . P . W e b b , " M e a s u r e m e n t s o f I o n i z a t i o n C o e f f i c i e n t s i n S i l i c o n a t L o w E l e c t r i c F i e l d s " , G E C a n a d a I n c .

    I n P : L . W . C o o k , e t . a l . , A p p l . P h y s . L e t t . 4 0 ( 7 ) , 1 A p r i l 1 9 8 2

    I n G a A s : T . P . P e a r s a l l , A p p l . P h y s . L e t t . 3 6 ( 3 ) , 1 F e b r u a r y 1 9 8 0

    G a A s : H . D . L a w a n d C . A . L e e , S o l i d - S t a t e E l e c t r o n i c s , 2 1 , 1 9 7 8

    2 0 0 3 0 0 4 0 0 5 0 0 0 . 1

    1

    1 0

    1 0 0

    1 0 0 0

    1 0 e 4

    1 0 e 5

    1 0 e 6

    Si (electron

    s)

    Ioni

    zatio

    n C

    oeffi

    cien

    ts[c

    m -1

    ]

    Ionization Coefficients for Semiconductors

  • - - - -

    + - - -

    - -

    - - +

    +

    - -

    - -

    + + + +

    P+ N+

    Si Multiplication Layer

    - - - + +

    - +

    - - + +

    - +

    - - + +

    - +

    - - +

    InP Multiplication Layer

    P+ N+

    The Avalanche Multiplication Process

  • Avalanche Photodiode Gain or Multiplication M

    Ionization coefficient ratio

    αe = Aexp(-B/E) Chyoweth's law

  • Avalanche Photodiode Gain or Multiplication M

    M = exp(αew) Ionization coefficient

    kwkkM

    e −−−−

    =])1(exp[

    Electrons only

    Electrons and holes

    k = αh / αe

  • Simplified schematic diagram of a separate absorption and multiplication (SAM) APD using a heterostructure based on InGaAs-InP. P and N refer to p and n -type

    wider-bandgap semiconductor.

    Heterojunction Photodiodes: SAM

  • Heterojunction Photodiodes: SAM

    (a)  Energy band diagrams for a SAM detector with a step junction between InP and InGaAs. There is a valence band step ΔEv from InGaAs to InP that slows hole entry into the InP layer.

    (b) An interposing grading layer (InGaAsP) with an intermediate bandgap breaks ΔEv and makes it easier for the hole to pass to the InP layer for a detector with a graded junction between InP and InGaAs. This is the SAGM structure.

  • Heterojunction Photodiodes: SAM

    Simplified schematic diagram of a more practical mesa-etched SAGM layered APD

  • SAM APDS: Need for Separate Absorption and Multiplication Regions

    Small bandgap avalanche regions tend to have large dark current.

    Absorption Region

    Multiplication Region

    e- e- e-

    Electric Field

    position

  • Electric Field Simulation for SHIP

    -600

    -500

    -400

    -300

    -200

    -100

    0

    100

    0.4 0.8 1.2 1.6 2

    Elec

    tric

    Fiel

    d [k

    V/c

    m]

    Distance into Detector [µm]

    Si InGaAs

    5 V 10 V 23 V

  • Gain and Dark Current vs. Bias. 23 µm diameter SHIP

    0.01

    0.1

    1

    10

    100

    0.1

    1

    10

    100

    1000

    10000

    0 5 10 15 20 25

    Gai

    n

    Dar

    k C

    urre

    nt [µ

    A]

    Reverse Bias [V]

    Theoretical Gain Measured Photocurrent Gain

  • 0.1

    1

    10

    1 10 100 1000

    3 dB

    Ban

    dwid

    th [G

    Hz]

    Gain

    SHIP Detector 3-dB Bandwidth versus gain

    315 GHz GB

  • Comparison of Acheivable GB Product for SHIP, SL, and InP APDs

    0

    100

    200

    300

    400

    500

    600

    700

    800

    0.1 1

    Gai

    n-B

    andw

    idth

    -Pro

    duct

    (GH

    z)

    Multiplication Layer Thickness [µm] 5

    SHIP APD SL APD

    InP APD

  • Staircase APD: Use of bandgap engineering to increase the ratio of ionization coefficients.