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The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

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Page 1: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

The Physics of Infrared Detectors(with a special emphasis on

MID-IR detectors)

Massimo Robberto

(ESA – STScI)

Page 2: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Outline

• Semiconductors as crystals

• Energy bands

• Intrinsic semiconductors

• Light on intrinsic semiconductors

• Extrinsic Semiconductors

• Impurity band conductors (IBC)

Page 3: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Periodic Table

Atomic structure: (four 2s2p) covalent bonds per atom

Page 4: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Crystal Structure: 2-d

simple cubic

Bravais lattice R ma nb pc

In two dimensions, there are five distinct Bravais lattices

Page 5: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Crystal Structure: 3-d

simple cubic body-centered cubic face centered cubic

In three dimensions, there are fourteen distinct Bravais lattices

A large number of semiconductors are cubic (a1=a2=a3= a “lattice constant”)

Page 6: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 7: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 8: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 9: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 10: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 11: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 12: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 13: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond Structure

Page 14: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Diamond StructureTwo interpenetrating face-centered cubic lattices

Diamond lattice:All same atoms (e.g. Si)

Zincblende lattice:different atoms in each sublattice(e.g.CdTe, GaAs)

Page 15: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Lattice planes in crystals: Miller indexes

Silicon and Germanium break on {1,1,1} planes

never confuse the spacing between lattice planes with the spacing between crystal planes

Page 16: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Example

The surface density of Silicon is

14 2

14 2

14 2

11.8 10 atoms/cm on {111}

9.6 10 atoms/cm on {110}

6.8 10 atoms/cm on {100}

Page 17: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Wigner-Seitz cellThe smallest (“primitive”) cell which displays the full symmetry of the lattice is the Wigner-Seitz cell.

Construction method: surfaces passing through the middle pointsto the nearest lattice points

In 3-d think to a polyhedron

Page 18: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Reciprocal lattice

g ha kb lc

The Bravais lattice after Fourier transform

real space reciprocal latticenormals to the planes(vectors) points spacing between planes 1/distance between points

(actually, 2/distance)

(distance, wavelength) 2k (momentum, wave number) Bravais cell Wigner-Seitz cell

Page 19: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Reciprocal lattice

Page 20: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Bragg conditionsWhen a wave impinges on a crystal - and it doesn't matter if it is an electromagnetic wave, e.g. X-rays, or an electron, or neutron "wave" - it will be reflected at a particular set of lattice planes {hkl} characterized by its reciprocal lattice vector g only if the so-called Bragg condition is met

k k g

If the Bragg condition is not met, the incoming wave just moves through the lattice and emerges on the other side of the crystal (neglecting absorption)

Page 21: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Elastic scattering

k k

For a given k, The Bragg conditions is met on surfaces normal to particular g.These surfaces define cells in the k-space, called

Brillouin zones

Page 22: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Brillouin Zone construction

All wave vectors that end on a BZ, will fulfill the Bragg condition and thus are diffracted. Wave vectors completely in the interior of the 1. BZ, or in between any two BZs, will never get diffracted; they move pretty much as if the potential would be constant, i.e. they behave very close to the solutions of the free electron gas.

Page 23: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

First BZ

Second BZ

Brillouin zoneThe Brillouin zone is defined in the reciprocal lattice.

The first BZ is the volume enclosed within a Wigner-Seitz cell in the k-space.

In 3-d think to a nested set of polyhedra

Third BZ

Page 24: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

WS zone and BZLattice Real Space Lattice K-space

bcc WS cell Bcc BZ (fcc lattice in K-space)

fcc WS cell fcc BZ (bcc lattice in K-space)

The WS cell of bcc lattice in real space transforms to a Brillouin zone in a fcc lattice in reciprocal space while the WS cell of a fcc lattice transforms to a Brillouin zone of a bcc lattice in reciprocal space.

Bcc: body-centered cubic; fcc: face-centered cubic

Page 25: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Brillouin zone of Silicon

Points of high-symmetry on the Brillouin zone have specific importance. The most important point for optoelectronic devices is the center at k = 0, known as the gamma point Γ. Note the points Γ, X, W, K,…

Page 26: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Wave vectors near or at a BZ - let's call them kBZ electrons - feel the periodic

potential of the crystal while the others do not. E.g., they are diffracted.

Page 27: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

ENERGY GAP in CRYSTALS

• On the BZ it is k=-k: these are two standing waves described by ~eikr and e-ikr

• Their combination can be symmetric

eikr+ e-ikr ~ cos(kr) or antisymmetric

eikr- e-ikr ~ sin(kr) • The probability density have different values at

each point• 2 different values of the energy, varying with k on the

BZ: ENERGY GAP.

Page 28: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

2

BZE(k ) = ± ( )2

kU g

m

Page 29: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Energy bands

22 ( ) ( ) ( )

2 k k kV r r E rm

If V(r) is periodic with periodicity of the lattice, then the wave Function is a plane wave (free electron) with periodic modulation

( ) ( , ) Block functionik rk nr e U k r

k is a wave vector in the reciprocal lattice, Un(k,r) is periodic in r, i.e. U(r+R)=U(r), and n is the band index.

-For a given n, it is sufficient to use k’s in the primitive cell of thereciprocal lattice (Brillouin zone). The rest is redundant!

F. Block solved the Shroedinger equation for an electron in thelattice:

Page 30: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Band Structure and Bloch’s Theorem

( ) ( , ) Block functionik rk nr e U k r

From:

It is also:( )( ) ( , ) ( )i K g r

k g n kr e U k g r r

Then:

( ) ( )E k g E k for dispersion curves that have a different origin

There are many energy values for one given k. In particular, all possible energy values are contained within the first Brillouin zone (between -1/2g1 and +1/2g1 in the

picture).

Page 31: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Band Structure and Bloch’s Theorem

reduced representation of the band diagram Every energy branch in principle should carry an index denoting the band (often omitted)

Energy functions of a periodic potentialThe electron at k1can go to the upperband if someone gives him 1. E > bandgap, AND 2. k2=kl+gTHIS IS THE BRAGGS LAW FOR

INELASTIC SCATTERING

Page 32: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Band diagram of Silicon

• Si has a band gap of about 1 eV.     • Si is an indirect semiconductor because the maximum of the valence band (at ) does not coincide with the minimum of the conduction band (to the left of X).

Page 33: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Direct and Indirect Semiconductors

Page 34: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Simplified band diagram

Conduction band

Valence band

Eg bandgap 1.24

( )cogE eV

Page 35: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Fermi Energy and Carrier Concentration

Density of electrons in the energy interval E, E + E = density of states probability for occupancy energy interval

The number (or density) of something is given by the density of available places times the probability of occupation.

( ) ( , )dN D E f E T dE

Page 36: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Density of states

2 2

2k

kE

m

A free (or under constant potential)particle in a rectangular box has:

1) only kinetic energy

2) k is discrete (stationary waves)

, , , ,

2x y z x y zk n

L

Therefore, the energy is quantized

22

2 2 22

2k x y zE n n nm L

kx

ky

kz

Page 37: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Density of states Ds

• In phase space a surface of constant energy is a sphere. The volume is

    •Any "state", i.e. solution of the Schroedinger equation with a specific k, occupies with 2 electrons the volume

• The number of cubes fitting inside the sphere at energy E thus is the number of all energy levels up to E:

34

3V k

32

kVL

3 3

22

3k

s

V k LN

V

3/ 21/ 2

3 2 2

1 1 2

2s

s

dN mD E

L dE

Finally:

Page 38: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Density of states Ds

At 0 K one can place electrons up to the Fermi level EF

3/ 21/ 2

2 2

1 2

2s

mD E

Page 39: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Probability of occupancy

FE-E

kT

1f(E,T)=

e 1

Fermi distribution

E – EF >> kT

Fermi level

Page 40: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Intrinsic Semiconductors

SiHgCdTe

InSb

Page 41: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

The concentration of electrons in the conduction band is

3/ 2 2

( ) ( , )c

F

Ee

E

E Ee KT

eff

Eg

KT

n D E f E T dE

N e

AT e

effective density of states at the band edge

3/ 2

2

24e e

effm kT

Nh

With A=4.831021 electrons m-3 K-3/2.The nr. of electrons in the conduction band depends on Eg and T.In Si ne doubles for ~8 degree rise in temperature

Page 42: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Same for the holes in the valence band:

ne = nh = ni “INTRINSIC CONCENTRATION”

And the mass action law is

3

3/ 22

2

24

gEi e p kT

e hkT

n n n e m mh

Eg(300 K) = 1.1242 eV

Eg(0 K) = 1.700 eV

The bandgap energy and the effective mass depend on T

for Silicon:

Page 43: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

The CONDUCTIVITY

e e h he n n

The mobility µ is the proportionality constant between the average drift velocity vD

of carriers in the presence of an electrical field E:

Dv EMobility depends on the average time between scattering processes

se

m

decreases with Eg. Leakage currents are lower in large Eg materials.

Page 44: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Radiation on intrinsic semiconductors

• at low T the conduction band is “empty”. Low intrinsic conductivity

• radiation with h>Eg creates electron-hole pairs: ne=nh

• both electrons and holes contribute to the photocurrent,depending on mobilities

• The conductivity changes: PHOTOCONDUCTOR

e e h h e e h he n n n n Where

ne,h = quantum efficiency) photon flux)

• all atoms count: absorption occurs in thin layer (~10micron)

Page 45: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Extrinsic semicondictorsSemiconductor

donorsacceptors

Doped semiconductors

Page 46: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

N-type and p-type

Page 47: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Ruby

The ruby mineral (corundum) is aluminum oxide with a small amount (about 0.05%) of chromium which gives it its characteristic pink or red color by absorbing green and blue light.

4.35ct avg 10mm red serengeti ruby, ACNTV PRICE $74.95 @ www.jewelrytelevision.com

Page 48: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

( , , )e eeff c Fn N f E E T

( , , )A A A FN N f E E T

1 ( , , )h heff V Fn N f E E T

1 ( , , )D D A FN N f E E T

e hA Dn N n N Charge neutrality

gives EF and therefore the concentrations

Page 49: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Extrinsic semiconductorsNormally : “Dopant or majority” vs. “ residual impurities”

Ex: Si:Ga (III group) is p-type Si:As (V group) is n-type• There are shallow- and deep-level impurities • shallow-level impurities increase the response• Atoms of dopant and residual impurities do not interact with each other.

• p-type: at low T the conduction band is “empty”; donor impurities have lost their electrons and are ionized, acceptor dopant has electrons from valence band and impurities; valence band has free holes.

D AN N

D AN ND AN N

Page 50: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Opposite requirements

To move away and collect charges we need an electric field:

To have a good drop of potential, no current must flow: Detector material must have high impedence

(I.e. low conductivity)

On the other hand, we want high concentration of absorbers: this goes in the direction of high conductivity

x

dVE

dx

Page 51: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Impurity band conduction

The donor band (As in Si:As ) can be heavily dopedPhotons are absorbed

• in thin layer (smaller volume)• providing higher QE• higher radiation immunity• lower applied bias• better uniformity• faster response

High dopant concentration creates a band ~1meV wide,thus the cutoff increasees from 24 to 28m.However:

The donor band becomes a conduction band:“Impurity Band Conduction”

Page 52: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Impurity band conduction

The donor band (As in Si:As ) is heavily dopedElectric field is applied (bias) and the free charge carriers are driven out from the IR active region (depletion):

High resistance and high electric field

Transparent contact (V+)

Blocking layer (intrinsic Si)

IR active region (heavily As doped)

Substrate (heavily doped n-type) at ground

Problem: charges “hop” in the impurity conduction band;If they are sensed there is an extra dark current: need for a blocking layer (BIB)

h+ e-

Page 53: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Photo-electrons and relative holes are collected

hole

Page 54: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Si:As Engeneering

• Dopant As is n-type. P-type impurities (e.g. B) are a potential problem

• They are “neutralized” by As, leaving them as negative charge centers in the “depletion region”

• These NA charges create an electric field that limits the extention of the depletion region w

Page 55: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

Poisson equation for the ionized impurities:

0 0 0 0

x AdE eN

dx k k

1/ 2

20 02b B B

A

kw V t t

eN

-tB

The width of the depletion region depends on the bias and on the impurity concentration

Assuming NA = 1012 cm-3 and Vb = 1V it is w=32m

Page 56: The Physics of Infrared Detectors (with a special emphasis on MID-IR detectors) Massimo Robberto (ESA – STScI)

An acceptable arsenic concentration is ND=3 x 1017 cm-3. For arsenic in silicon, the absorption cross section is Si:As= 2.2 x 10-15 cm2

the absorption length is l=1/ ND Si:As = 15m.

Since l<w, a high quantum efficiency detector can be built.

Most of the failures in detector processing have to do with unwanted impurities, and the improvement of the performance of this detector type is closely linked to driving down NA.

Spitzer Si:As (BIB)128x128 array