Atomic and Molecular Physics 2: Solutions for PC 4243, Exams of Solid State Physics

Solutions for various questions related to atomic and molecular physics 2 (pc 4243) as taught in the academic year ay06/07, semester 2. Topics covered include hyperfine splitting, ionization energy, selection rules, linewidths, doppler shift, and entropy. Students can use these solutions as a reference for understanding the concepts and solving related problems.

Typology: Exams

2012/2013

Uploaded on 02/20/2013

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PC 4243 - Atomic and Molecular Physics 2
AY06/07 SEM 2
Suggested Solutions
The use of Prof Christian’s official solutions as reference is acknowledged.
Q1
a (i)
Li has 3 electrons, and its complete electronic configuration is 1s22s, with spec-
troscopic notation 2S1/2.
b
The levels in the P and D column appear in pairs because of the spin-orbit
interation.
1
pf3
pf4
pf5

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PC 4243 - Atomic and Molecular Physics 2

AY06/07 SEM 2

Suggested Solutions

The use of Prof Christian’s official solutions as reference is acknowledged.

Q

a (i)

Li has 3 electrons, and its complete electronic configuration is 1s^22 s, with spec- troscopic notation 2 S 1 / 2.

b

The levels in the P and D column appear in pairs because of the spin-orbit interation.

c

The hyperfine interaction leads to a splitting of the ground state.

For 7 Li with I = 3/ 2 , J = S = 1/2, F = 1, 2, so that EHF S = A/2(F (F +1)− J(J + 1) − I(I + 1)) gives EHF S = 3/ 2 A for F = 2 and EHF S = − 3 / 4 A for F = 1.

For 6 Li with I = 1, F = 3/ 2 , 1 /2 with corresponding values of EHF S = A/ 2 A and −A respectively. The physical origin of the hyperfine splitting is due to the contact interaction of s-electrons at the location of the nucleus.

d

The ground state splitting between the 2 levels are given by

∆EHF S =

A

[(F +(F +^ + 1) − J(J + 1) − I(I + 1)) − ((F +^ − 1)(F +) − J(J + 1) − I(I + 1))]

A

F +

where F +^ denotes the larger F value. Now A ∝ gI so that ∆EHF S ∝ gI F +, and we have

g^6 I =

∆E^6 HF S

∆E^7 HF S

F +

F +

e

The ionisation energy is proportional to the reduced mass, so that

E 1 = E 2 μ 1 μ 2

with

μ 1 = meMi Mi + me = me

me Mi + me

≈ me

me Mi

Q

a

λ =

Ee − Eg

62350cm−^1 − 44043cm−^1 = 18307cm−^1

b

(^3) P 2 means S = 1, L = 1, J = 2. 3 S 1 means S = 1, L = 0, J = 1. Yes, the

transition follows the common selecton rules for dipole transition as ∆L = 1.

c

The homogenous linewidth is due to exponential decay :

A(t) = eiω^0 t^ · e−t/^2 τ

whose fourier transform

a(ω) =

ei(ω^0 −ω−^1 /^2 τ^ )t^ dt

=

i(ω − ω 0 ) − 1 / 2 τ |a(ω)|^2 =

(ω − ω 0 )^2 + (1/ 2 τ )^2

Thus the FWHM δω = 2 (^21) τ = (^) τ^1 , giving

δfF W M H =

2 π

τ = 19.89MHz

d

The Doppler shift is given by ∆f = v¸, so thatf

v = ∆f c f

= ∆f λ

. Assume a velocity distribution

p(vx) ∝ e−^

(^12) mv (^2) x/kT = e−^

∆ 2 σf 22

with

σ =

kT m

λ

. To find the Half Width at Half Maximum, we set

1 2 = e−^

x^2 2 σ^2

⇒ ln

x^2 2 σ^2 ⇒ x = σ

2 ln 2

so that

∆fF W HM = 2

2 ln 2σ

= 2

2 ln 2

kT m

λ = 495 .99MHz

e

From P V = N kT we define the number density

ρ =

N

V

P

kT

. For hard core collisions, the collisional cross sectional area σ = D^2 π.

From kinetic theory, the mean velocity v =

2 kT m. The mean free path s = (^) σρ^1 = (^) P DkT (^2) π , so that the mean time between collisions

t = s v = kT P πD^2

m 2 kT

=

P πD^2

kT m 2 = 8. 6 × 10 −^5 s−^1

Then ∆f =

t = 11.6kHz.

Q

a

The interaction Hamiltonian

H(t) = B〈F = 4|μˆ|F = 3〉

where ˆμ = ˆμs = gs sˆz μB /ℏ. Here,

|F = 3〉 =

(|mi = 1/ 2 , mj = − 1 / 2 〉 + |mi = − 1 / 2 , mj = 1/ 2 〉)

so that

〈 4 |μˆz | 3 〉 =

gs(〈− 1 | − 〈+|)ˆμz (|−〉 + |+〉)

=

gs(〈−|sz |−〉 − 〈+|sz |+〉)

=

gsμB (−hbar/ 2 − ℏ/2)

= gs μB ℏ

= μB

Now

ℏΩR = B 0 μB ⇒ ΩR =

B 0 μB ℏ so that

B 0 =

ΩR

μB

2 πfR μB

= 7. 14 × 10 −^8 T

b

ρe =

Ω^20

Ω^20 + ∆^2

12 + 2^2

c

No, because √^12 (〈−|±〉 + |) is an eigenstate of ˆsx = 12 (ˆs+ + ˆs−) so 〈−|sˆx|+〉 = 0 implying no transfer.