Derivations Flashcards

1
Q

Derive the reduced mass if

-ℏ^2/2me ∇^2e Ψ(re,rn) - ℏ^2/2mn ∇^2n Ψ(re,rn) + V(re-rn) Ψ(re,rn) = Etotal Ψ(re,rn)

A

R + (X,Y,Z) = 1/M (me xe + mn xn…)

r = (x,y,z) = re - rn = (xe - xn…)

M = me + mn

chain rule for d/dxe and d/dxn

square both sides

substitute into Schrodinger equation

mixed derivatives cancel

giving as required with definition of reduced mass defined

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2
Q

use separation of variables for Ψ(re,rn) = Ψ(r)Φ(R)

to solve

ℏ^2/2M ∇^2 Ψ(re,rn) - ℏ^2/2μ ∇^2 Ψ(re,rn) + V(re-rn) Ψ(re,rn) = Etotal Ψ(re,rn)

A

first term corresponds to R and second r. So they attach to derivative.

Divide by Ψ(r)Φ(R) and identify the first term as ECoM and second term as E

such that EcoM + E = Etotal

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3
Q

use separation of variables for Ψ(r,θ,Φ) = R(r)Y(θ,Φ) to solve

eq.1.30

A

substitute into eq.1.30 where r corresponds to first term and θ,Φ the second term.

multiply by r^2/RY and rearrange to find the terms independent of r and terms independent of
θ,Φ.

Term independent of r is l(l+1)

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4
Q

use separation of variables for Y(θ,Φ) = Θ(θ)Φ(ϕ) to solve

eq. 1.36

A

substitute into eq. 1.36 and multiply by sin^2θ/ΘΦ

find the term independent of θ and the term independent of ϕ

where the term independent of θ is the constant m^2

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5
Q

Solve the Legendre differential equation (eq. 2.7) by using the taylor series

Θ(x) = (∞∑k=0) ck x^k

A

set m = 0 and divide by sin^2 = 1-x^2

substitute the taylor series in and take the derivative.

Expand the brackets and take the derivative

shift k such that each x term is x^k

collect like terms

set equal to zero and rearrange for ck+2

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6
Q

solve the associated legendre differential equation eq.2.7

using the substitution

Θ = (1 − x^2)^m/2 y

A

here m does not equal 0

use the product rule

and substitute into the legendre differential equation

divide through by (1 − x^2)^m/2 y gives the transformed equation

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7
Q

Solve the Laguerre differential equation (eq.2.50) by using the taylor series

L(p) = (∞∑k=0) ck p^k

A

substitute the series into eq. 2.50

take the derivatives and collect like terms

shift ck by 1 so that they are all to the power of p^k

which gives the recursion relations for ck

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8
Q

Solve the centrifugal barrier eq.3.10 through change of variables

A

change the dependent variable R(r) = U(r)/r and divide through by r

we can identify Veff(r) = V(r) + ℏ^2/2µ l(l+1)/r^2

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9
Q

Find the constants of proportionality Clm and Dlm

A

L+ |l,ml > = Clm|l,ml+1>
L- |l,ml > = Dlm|l,ml-1>

unit normalise (mod square)

replace with definitions of L+ and L-

expand brackets and replace with with operator eigenvalues

giving as required

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10
Q

derive L.S

A

J = L + S
J^2 = (L+S)^2
J^2 = L^2 + S^2 + 2L.S
L . S = 1/2(J^2-L^2-S^2)

or L.S = L+S- + L-S+ + 2LzSz

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11
Q

Calculate the corrections of pertubation

A

H(λ) = Hˆ(0) + λHˆ(1)
H(λ)|n(λ)⟩ = En(λ)|n(λ)⟩

where n(λ) and En(λ) are a taylor series of |n^(0)> + λ|n^(1)> …

substitute into H(λ)|n(λ)⟩ = En(λ)|n(λ)⟩

multiply out each term and collect like factors of λ

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12
Q

Derive the relativistic correction based on its Hamiltonian eq.5.10

A

H^(0) = p^2/2me - Ze^2/r4πϵ0r

rearrange for p^2/2me and substitute

calculate the first order pertubation

replace H^(0) with En^(0) and expand brackets

divide through by (En^(0))^2 and substitute in 1/r and 1/r^2

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13
Q

Derive the spin orbit correction based on its Hamiltonian eq. 5.15

A

substitute L.S based on J^2 = (L+S)^2

calculate first order pertubation

put in 1/r^3 and L^2, S^2 and J^2

which gives two solutions for j

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14
Q

Derive the total fine structure corrections

A

Add together Erel + Eso if l ≠ 0

then Erel + Edar if l = 0

Adding all three gives one whatever the l.

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15
Q

Derive the electric dipole selection rules

if [Lz,z] = 0, {P,z} = 0 and [L^2,[L^2,z]] = 2h^2(L^2z + zL^2)

A

0 =! <n,l,ml | … |n’,l’,ml’>

start with first relation giving ml = ml’

second relation states parity must change

and third that ∆l = |l −l’| =0

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16
Q

Derive the lande g factor for a weak magnetic field

A

Hzeeman = ωL(Lz + 2Sz)

use JJ states for first order pertubation

we get Ezeeman = ℏωL (l+2s)

using a general rule <Sz> -= κ<Jz></Jz></Sz>

redo first order calculation

giving κ+1 = g

17
Q

derive the L-S coupling regime selection rules

A

Jinit = Jfinal + Jph

and Jph = 1

so |∆J| = 0, 1

using the electric dipole from the stark effect hamiltonian

we get |<f|Hdipole|i>|^2 where [S^2,r] = 0 and [S^2,Hdipole] = 0

such that |∆S| = 0

therefore if we have the first two rules |∆L| = 0, 1

18
Q

Starting with eq 10.1 rewrite the hamiltonian using R and r

A

R = 1/2(r1+r2) and r = (r1-r2)

in terms of m1 and m2 this time

M = m1+m2

d/dx1 and d/dx2 can be found as before

square it and substitute into the schrodinger equation replacing for µ =1/2me

19
Q

using separation of variables

Ψ(r1,r2) = ψCoM(R)ψrel(r) to solve C.2

A

substitute in the variable and divide through by
ψCoM(R)ψrel(r)

recognise that the first term is ECoM and second is E

giving as required

20
Q

using separation of variables

ψrel(r) = ψvib(r)ψrot(θ, ϕ)

to solve C.9

A

Use spherical polar coordinates

substitute in and multiplying through by r^2

we can regonise that the first term is -Erot,r0^2

and the second Erot,r0^2

21
Q

Starting from equation 10.11 derive the vibrational modes

A

r = r0 such that r = r0 + x

d/dx (d/dx ψvib)&raquo_space; 1/r0 (d/dx ψvib)

hence neglect the second term

Veff is a taylor expansion where E absorbs V(r0) and V’ = 0

V’’ = k

22
Q

show that [a+,a-] = -1

A

use commutator relation and substitute in

23
Q

calculate the expectation values of a+ and a-

A

exact same as L+ and L-

use coefficients Bn and An

unit normalise and substitute in known expressions