Schrodinger Equation in Three Dimensions Flashcards

1
Q

Schrodinger Equation in 3D

Time Dependent

A

iℏ ∂ψ(|r,t)/∂t= -ℏ²/2m ∇²ψ(|r,t) + V(|r,t)ψ(|r,t)

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2
Q

Schrodinger Equation in 3D

Probability Density

A

ψ(|r,t) |²

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3
Q

Schrodinger Equation in 3D

Normalisation

A

∫ | ψ(|r,t) |² dV = 1

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4
Q

Schrodinger Equation in 3D

Time Independent

A
  • ℏ²/2m ∇²ψ(|r) + V(|r)ψ(|r) = E ψ(|r)

- i.e. V=V(|r) => ψ(|r,t) = ψ(|r) * e^(-itE/ℏ)

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5
Q

3D Infinite Potential Well

Description

A
  • consider a box with no potential inside (V=0) and infinite potential outside (V=∞)
  • solve the Schrodinger equation inside the box and then impose the condition that solutions must be zero at the walls of the box, i.e standing waves in the box
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6
Q

3D Infinite Potential Well

Proof

A

-the potential is time independent so the Schrodinger equation takes the form:
-ℏ²/2m ∂²ψ(|r)/∂x² - ℏ²/2m ∂²ψ(|r)/∂y² - ℏ²/2m ∂²ψ(|r)/∂z²
= E ψ(|r)
-different coordinates appear independently so seek solution of the form:
ψ(|r) = F(x)G(y)H(z)
-sub into the Schrodinger equation
-this gives rise to 3 equations:
d²F/dx² * 1/F + FCx = 0
=> Enx = nx²
ℏ²π²/2mLx² , nx = 1,2,3,…
Fnx(x) = [2/Lx]sin(nxπx/Lx)
-and similarly for y and z
-total energy:
E = Enx + Eny + Enz
= ℏ²
π²/2m * [nx²/Lx² + ny²/Ly² + nz²/Lz²]
-total wave function:
ψ(|r) = F(x)G(y)H(z)
= √[8/LxLyLz]sin(nxπx/Lx)sin(nyπy/Ly)sin(nzπ*z/Lz)

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7
Q

Degeneracy of the Energy Spectrum

1D

A

-in the 1D case:
En = ℏ²π²n²/2mL²
-for each En, there exists a unique wave function:
φ(x) = √[2/L] * sin(πnx/L)
-one wave function per energy level, no degeneracy

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8
Q

Degeneracy of the Energy Spectrum

3D

A
  • different combinations of nx, ny and nz can have the same energy but different wave functions
  • in the 3D case, SOME energy states are degenerate, this is due to symmetry of the well
  • when the symmetry breaks, degeneracy is removed
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9
Q

Schrodinger Equation for a Central Potential

A

[^K+^U] ψ(|r) = Eψ(|r)

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10
Q

Hydrogen Atom

^K

A

^K = -ℏ²/2m [∂²/∂x² + ∂²/∂y² + ∂²/∂z²]

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11
Q

Hydrogen Atom

|^L²

A

|^L² = -ℏ²[1/sinθ ∂/∂θ(sinθ∂/∂θ) + 1/sin²θ ∂²/∂φ²]

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12
Q

Hydrogen Atom

Schrodinger Equation

A
  • ℏ²/2m [1/r ∂/∂r (r² ∂/∂r) - 1/ℏ²r² |^L]*ψ(|r) + U(r)ψ(|r) = Eψ(|r)
  • > where U(r) = -e²/(4πϵo*r)
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13
Q

Angular Momentum

Classical vs Quantum

A
-in classical physics:
|L = |r x |p
-in quantum mechanics:
|^L = |^r x |^p
^Lx = ^y^pz - ^z^py
^Ly = ^z^px - ^x^pz
^Lz = ^x^py - ^y^px
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14
Q

Can the three quantum angular momentum operators ^Lx, ^Ly, ^Lz be measured simultaneously?

A

-operators can be measure simultaneously IF [^A,^B]=0
-but:
[^Lx , ^Ly] = -iℏ^Lz
[^Ly , ^Lz] = -iℏ^Lx
[^Lz , ^Lx] = -iℏ^Ly
-therefore we cannot measure all three components of angular momentum at the same time

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15
Q

Eigenvalue Problem of ^|L

A
-define ^|L² = Lx² + Ly² + Lz²
=>
[^Lz , ^|L²] = 0
[^Ly , ^|L²] = 0
[^Lx , ^|L²] = 0
-this means we can pick one component e.g. ^Lz and diagonalise it together with ^|L²
-the common eigenvectors of these two operators are:
{ |l*ml⟩ }
-corresponding eigenvalues:
^|L² |l*ml⟩ = ℏ²l(l+1) |l*ml⟩
^Lz |l*ml⟩ = ℏm |l*ml⟩
-therefore we need two numbers to label the eigenvalues and eigenvectors of these operators, l and ml
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16
Q

Possible Values of l and ml

A

l = orbital quantum number, must be an integer
ml = azimuthal quantum number takes values in the interval -l to l inclusive
e.g. l=0 => ml = 0
l=1 => ml = -1,0,1
l=2 => ml = -2,-1,0,+1,+2
etc.

17
Q

Spherical Harmonics

A

-in coordinate representation, the eigenvectors of angular momentum are known as spherical harmonics:
⟨ θ , φ|l*ml⟩ ⟩= Ylml(θ,φ)
-the spherical harmonics also solve the eigenvalue problem Av=λv, v = Ylml
-and they are orthonormal

18
Q

What is ml graphically?

A

-ml is equal to the number of nodes in the interval 0 to 2π of φ

19
Q

The Radial Equation

A

-starting with the Schrodinger equation for the Hydrogen atom, assume a solution of the form:
ψ(|r) = R(r)*Ylml(θ,φ)
-sub in and cancel Y terms to arrive at the radial equation;
-ℏ²/2m 1/r d/dr (r² dR(r)/dr) - ℏ²l(l+1)/2mr² R(r) + U(r)R(r) = ER(r)

20
Q

Solutions of the Radial Equation

A

-allowed energies are quantised in terms of radial quantum number, n:
En = - C 1/n²
-where C is a constant, C = me^4/2(4πϵo)²ℏ²

21
Q

What are the allowed quantum numbers for the electron inside the hydrogen atom?

A
n = 1, 2, 3, ....
l = 0, 1, 2, ... , n-1
ml = -l, .... , +l
22
Q

Quantum Number

Definition

A

-an eigenvalue of some operator ^O which commutes with ^H, [^H,^O]=0, i.e. they will not change as time goes on so can always be used to specify the state of the system

23
Q

l and shells

A
l=0 => l=s
l=1 => l=p
l=2 => l=d
l=3 => l=f
...
24
Q

Hydrogen Wave Functions

A

-the total wave function of the hydrogen atom:
ψ(|r) = Rnl(r) Ylml(θ,φ)
-radial wave functions are found by solving the radial equation, and they are normalised by:
∫ r² |Rnl(r)|² dr = 1
-where the integral is from 0 to infinity

25
Q

Hydrogen Atom

Level Degeneracy

A

-similar to the 3D potential well, for the hydrogen atom we also find degeneracy of certain levels:
-total degeneracy of level n is:
gn = n²

26
Q

Hydrogen Atom

Electron’s Whereabouts

A
  • probability density is a cloud, i.e the electron is smeared out over some region of space
  • as n increases, the probability extends further from the nucleus
  • in s states (l=0) probability is spherically symmetric
  • in p states (l=1) one possible orbit is along the z-axis and 2 in the x-y plane
  • in all state l>0, probability density vanishes at the origin
27
Q

Radial Probability

A

-when the atom is isolated from external fields, it has spherical symmetry
-the probability of finding an electron doesn’t depend on angle but does depend on radial distance:
probability of finding electron at distance r
= r² |Rnl(t)|²