Materials Science and Engineering/Derivations/Semiconductor Devices

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pn Junctino Electrostatics

Effect of an Electric Field - Conductivity and Ohm's Law

 E=UL

a=emE

vaverage=aτ

vD=(emτ)E

J=NeevD

J=Nee2τmE

J=σE

σ=(emτ)(Nee)

 σ=μe(Nee)

The Built-in Potential (Vbi)

The electric field is the derivative of the potential with position

E=dVdx

Integrate across the depletion region

xpxnEdx=V(xp)V(xn)dV=V(xn)V(xp)=Vbi

The sum of the drift and the diffusion at equilibrium is equal to zero

JN=qμNnE+qDNdndx=0

Use the Einstein relationship:

E=DnμNdn/dxn=kTqdn/dxn

Vbi=xpxnEdx=kTqn(xp)n(xn)dnn=kTqln[n(xn)n(xp)]

ND and NA are the n- and p-side doping concentrations.

n(xn)=ND

n(xp)=ni2NA

 Vbi=kTqln(NANDni2)

Depletion Width

Solution of charge density

Solution of electric field

Solution of V

Solution of xn and xp

Depletion Width with Step Junction and VA not equal to zero

File:Pn junction electrostatics.png

pn Junction Diode: I-V Characteristics

Assumptions

  1. Diode operated in steady state
  2. Doping profile modeled by nondegenerately doped step junction
  3. Diode is one-dimensional
  4. In quasineutral region the low-level injection prevails
  5. The only processes are drift, diffusion, and thermal recombination-generation

General Relationships

I=AJ

J=JN(x)+Jp(x)

JN=qμnnE+qDNdndx

Jp=qμppEqDpdpdx

Quasineutral Region Consideration

The quasineutral p-region and n-region are adjacent to the depletion region

0=DNd2Δnpdx2Δnpτn

0=DPd2Δpndx2Δpnτp

The electric field is zero and the derivative of the electron and hole concentration is zero in the quasineutral regions.

JN=qDNdΔnpdx

JP=qDPdΔpndx

Depletion Region

Continuity equations:

0=1qdJNdx+nt|thermalRG

0=1qdJPdx+pt|thermalRG

Assume that the thermal recombination-generation is zero throughout depletion region. Sum the JN and JP solutions.

J=JN(xp)+JP(xn)

Strategy to find the minority carrier current density in the quasineutral regions:

  • Evaluate current densities at the depletion region edges
  • Add edge current densities
  • Multiply by A to find the current

Boundary Conditions

Ohmic Contacts

Δnp(x)=0

Δpn(x+)=0

Depletion Region Edge

Establish boundary conditions at the edges of the depletion region.

Multiply defining equations of the electron quasi-Fermi level, FN, and the hole quasi-Fermi level, FP.

np=ni2e(FNFP)/kT

Monotonic variation in levels

FNFPEFnEFp=qVA

"Law of Junction"

np=ni2eqVA/jT

Evaluate the "law of junction" at the depletion region edges to find the boundary conditions.

n(xp)p(xp)=n(xp)NA=ni2eqVA/kT

n(xp)=ni2NAeqVA/kT

 Δnp(xp)=ni2NAeqVA/kT1)

n(xn)p(xn)=p(xn)ND=ni2eqVA/kT

p(xn)=ni2NDeqVA/kT

 Δpn(xn)=ni2ND(eqVA/kT1)

Derivation

  1. Solve minority carrier diffusion equations with regard to the boundary conditions to determine value of Δnp and Δpn in quasineutral region.
  2. Determine the minority carrier current densities in quasineutral region
  3. Evaluate quasineutral region solutions of JN(x) and JP(x). Multiply result by area

Solve the equation below with regard to two boundary conditions.

0=DPd2Δpndx'2Δpnτp

Δpn(x)=0

Δpn(x=0)=ni2ND(eqVA/kT1)

General solution:

Δpn(x)=A1ex/LP+A2ex/LP

LP=DPτP

 Δpn(x)=ni2ND(eqVA/kT1)ex/LP
 JP(x)=qDPdΔpndx=qDPLPni2ND(eqVA/kT1)ex/LP
 Δnp(x)=ni2NA(eqVA/kT1)ex/LN
 JN(x)=qDNdΔnpdx=qDNLNni2NA(eqVA/kT1)ex/LN

Evaluate at the depletion region edges

JN(x=xp)=JN(x=0)=qDNLNni2NA(eqVA/kT1)

JP(x=xn)=JP(x=0)=qDPLPni2ND(eqVA/kT1)

Multiply the current density by the area:

I=JA=qA(DNLNni2NA+DPLPni2ND)(eqVA/kT1)

Ideal diode equation:

 I=I0(eqVA/kT1)
 I0=qA(DNLNni2NA+DPLPni2ND)

The Effective Mass

Derivation 1

The velocity of an electron in a one-dimensional lattice is in terms of the group velocity

vg=1Ek

dE=eEvgdt

dE=eE1Ekdt

Differentiate the equation of velocity

dvgdt=1ddtEk

dvgdt=12Ek2dkdt

dvgdt=122Ek2eE

mdvdt=eE

 m*=2(2Ek2)1

Derivation 2

In the free electron model, the electronic wave function can be in the form of eikz. For a wave packet the group velocity is given by:

v=dωdk = 1dεdk

In presence of an electric field E, the energy change is:

dε=dεdkdk=eEdx=eEvdt=eEdεdkdt

Now we can say:

dkdt=dpdt=mdvdt

where p is the electron's momentum. Just put previous results in this last equation and we get:

mdkdt=1ddtdεdk=1d2εdk2dkdt

From this follows the definition of effective mass:

1m=12d2εdk2

The Zimman Model

Wavefunction:

Ψk=eikx

Strong disturbance when individual reflections add in phase

nλ=2asinθ

k=nπa

Ψk=eikx

Ψ±=12(eikx±eikx)=2[coskxisinkx]

The potential energy is from the actual potential V(x) weighted by the probability function |Ψ±|2

V±=1L|Ψ±|2V(x)dx

V±=1L[2cos2kx2sin2kx]V(x)dx

Average over one period

V±=1a0a[2cos2kx2sin2kx]V(x)dx

V±=1a0a[1+cos2kx1+sin2kx]V(x)dx

±1a0acos2kxV(x)dx

V±=±Vn

The kinetic energy is the same in the case of both wave functions

E=2k22m

The total energy is the kinetic energy plus the potential energy

E±=2k22m±Vn

The energy of an electron cannot be between the lower and higher value.