Materials Science and Engineering/Doctoral review questions/Discussion List

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Discussion List

  • Definition of a mode (i.e., for optical fibers) (Melissa Smith)
  • Quantum mechanical descriptions of electron (Megan)
    • Free electron
    • Infinite well
    • Finite well
    • Harmonic oscillator
    • Hydrogen (H)
    • Hydrogen (H2)
      • Hartree Fock
  • Fermi energy, occupation levels for electrons
  • Photonic Bandgap and Periodic Mediums (George)

Wave equation

A pulse traveling through a string with fixed endpoints as modeled by the wave equation.

Electromagnetic waves as a general phenomenon were predicted by the classical laws of electricity and magnetism, known as Maxwell's equations. If you inspect Maxwell's equations without sources (charges or currents) then you will find that, along with the possibility of nothing happening, the theory will also admit nontrivial solutions of changing electric and magnetic fields. Beginning with Maxwell's equations for a vacuum:

𝐄=0  (1)
×𝐄=t𝐁(2)
𝐁=0  (3)
×𝐁=μ0ϵ0t𝐄   (4)
where
is a vector differential operator (see Del).

One solution,

𝐄=𝐁=𝟎,

is trivial.

To see the more interesting one, we utilize vector identities, which work for any vector, as follows:

×(×𝐀)=(𝐀)2𝐀

To see how we can use this take the curl of equation (2):

×(×𝐄)=×(𝐁t)   (5)

Evaluating the left hand side:

×(×𝐄)=(𝐄)2𝐄=2𝐄 (6)
where we simplified the above by using equation (1).

Evaluate the right hand side:

×(𝐁t)=t(×𝐁)=μ0ϵ022t𝐄(7)

Equations (6) and (7) are equal, so this results in a vector-valued differential equation for the electric field, namely

2𝐄=μ0ϵ02t2𝐄

Applying a similar pattern results in similar differential equation for the magnetic field:

2𝐁=μ0ϵ02t2𝐁.

These differential equations are equivalent to the wave equation:

2f=1c22ft2
where
c is the speed of the wave and
f describes a displacement

Or more simply:

2f=0
where 2 is d'Alembertian:
2=21c22t2=2x2+2y2+2z21c22t2 

Notice that in the case of the electric and magnetic fields, the speed is:

c=1μ0ϵ0

Which, as it turns out, is the speed of light. Maxwell's equations have unified the permittivity of free space ϵ0, the permeability of free space μ0, and the speed of light itself, c. Before this derivation it was not known that there was such a strong relationship between light and electricity and magnetism.

Snell's Law

Wavefronts due to a point source

In optics and physics, Snell's law (also known as Descartes' law or the law of refraction), is a formula used to describe the relationship between the angles of incidence and refraction, when referring to light or other waves, passing through a boundary between two different isotropic media, such as air and glass. The law says that the ratio of the sines of the angles of incidence and of refraction is a constant that depends on the media.

Named after Dutch mathematician Willebrord Snellius, one of its discoverers, Snell's law states that the ratio of the sines of the angles of incidence and refraction is equal to the ratio of velocities in the two media, or equivalently to the inverse ratio of the indices of refraction:

sinθ1sinθ2=v1v2=n2n1

Derivation

Incident, Reflected, and Transmitted Wave

File:Angles of incidence, reflection, and transmission.png

Equations of wave resulting from movement initially from left to right:

Incident Wave: Eieωtikir

Reflected Wave: Ereωtikrr

Transmitted Wave: Eteωtiktr

Boundary Equations

Dispersion relations with regard to a homogeneous medium provide the following equations:

|ki|=|kr|=ωn1c

|kt|=ωn2c

The phases of the field be equal in order that the boundary conditions are satisfied.

(k1r)x=0=(k1r)x=0=(k2r)x=0

(k1yy+k1zz)=(k1yy+k1zz)=(k2yy+k2zz)

k1y=k1y=k2y
k1z=k1z=k2z

The vector r is an arbitrary vector in the z-y plane.

r=(x=0,y,z)=rzy

(k1trt)=(k1trt)=(k2trt)

The vectors k1,k1,k2 are all in the plane of incidence. The coordinate system is oriented such that the plane of incidence is the same as the x-z plane.

E=Eei(ωtkxxkzz)

The tangential components of the wavevector are the same regardless of the medium is lossless of absorbing

k1z=k1z=k2z=β

kiz=ktz|ki|sinθ1=|kt|sinθ2

ωn1csinθ1=ωn2csinθ2

Conclusion of Derivation

Angle of reflection is equal to angle of incidence:

 θi=θr

Snell's law:

 n1sinθ1=n2sinθ2

Density of States for 1D, 2D, 3D

System

N electrons in box of side length L

Hamiltonian

H^(r1,r2,...,rN)=i=1N22mi2

H^(r1,r2,...,rN)=i=1NHi^

Eigenvalues and Eigenfunctions

H^iuk(x,y,z)=Ekuk(x,y,z)

uk(x,y,z)=uk(r)

1V1/2eikr

ϵk=2(kx2+ky2+kz2)2m

Born Von-Karman Boundary Conditions

uk(x+L,y,z)=uk(x,y,z)

uk(x,y+L,z)=uk(x,y,z)

uk(x,y,z+L)=uk(x,y,z)

k vectors

  • k vector: momentum
  • Energy eigenfunctions: momentum eigenfunctions
P^uk(r)=iuk(r)
P^uk(r)=kuk(r)
  • The k vector can be interpreted as a wave vector
|k|=2πλ
  • λ: de Broglie wavelength

Boundary Conditions

  • Apply boundary condition to develop identities
eikxL=eikyL=eikzL=1
  • The boundary conditions result in quantization of k vectors
kx=2πnxL
ky=2πnyL
kz=2πnzL
ϵk=2(2π)3(nx2+ny2+nz2)2mL2

Enumerate States

File:Ky - kx space.png
  • Nspatialstates=Ω(2πL)2
  • Nspatialstates=(L2π)2
  • Nspatialstates=DOS×area
(L2π)2: density of spatial states in k space

Fermi Surface

After introducing electrons into the system, what states will they occupy? Lowest energy levels are filled, and the Fermi surface, which is a circle in 2D and a sphere in 3D, separates the filled from unfilled states.

  • Nelectrons=22πkF331(2πL)3
  • Nelectrons=24πkF33V(2π)3

The number of electrons per unit volume, n, is equal to the total number of electrons, Nelectrons, divided by the volume:

  • n=NV
  • n=kF33π2

Fermi energy

The Fermi energy is typically between 1.5eV and 15eV

  • ϵF=22mkF2

Ground State Energy

  • E=2kkF22mk2
  • E=k<kFd3kV8π322mk2
  • E=Vπ22kF510m

Energy per electron:

  • EN=35ϵF

Density of States

The density of states is used to determine how many states are in the interval ϵϵ+dϵ

The number of states provided in the free electron case is as expressed below:

  • N=24πk331(2πL)3
  • N=(2mϵ2)3/2

The density of states is the derivative of the number of electrons with respect to ϵ:

  • dNdϵ=g(ϵ)
  • dNdϵ=m2π22mϵ2

The number of energy levels in the range ϵϵ+dϵ is the density of states multiplied by dϵ:

  • g(ϵ)dϵ

The density of states in a particular band is expressed below:

  • gn(ϵ)=14π3Sn(ϵ)dS|kϵ(k)|
  • g(ϵ)=ngn(ϵ)

Bloch Theorem

Periodic Potential and Expression with Fourier Series

V(r+T)=V(r)

T: Translation vector of the lattice
 V(r)=GVGexp(iGr))
G: sum over all reciprocal vectors
VG: Fourier coefficients of the potential
G: Reciprocal lattice vector

Expression of Wave Function with Fourier Transformation

 Ψ(r)=kCkexp[ikr]
Ck: Fourier coefficients of the wave function
k: Wave vectors

k vectors

 kx=±nx2πNa
2πa: magnitude of reciprocal lattice vector
nx2πa: whole set of reciprocal lattice vectors
1N: intersperse N points between reciprocal lattice points

Connection between wave vectors and reciprocal vectors

Express any wave vector, k, as the sum of a reciprocal vector, G, and wave vector that is within the Brillouin zone.

 k=G+k
k: wavevector always confined to the Brillouin zone of the reciproval lattice

Substitute expressions into the Schrodinger equation

[222m+V(r)]Ψ=EΨ

 k(k)22mCkexp(ikr)+kGCkVGexp(i[k+G]r=EkCkexp(ikr)

Rename the summation indices and replace k

k+G=k

k=kG

V(r)Ψ=G,kVGCkGeikr

keikr[(2k22mE)Ck+GVGCkG]=0

The equation is true with regard to an space vector r

 ((k)22mE)Ck+G(CkGVG)=0

The known Fourier coefficients of the periodic potential are coupled to the Fourier coefficients of the wave function.

[2m(kG)2V0V2mk2V0V2m(k+G)2][CkGCkCk+G]=Ek[CkGCkCk+G]

de Broglie Relation

 E=hf=ω

ω=12mvg2

ωk=mvgvgk

=mvgk

k=mvg

 λ=hmvg