Note that this was just a classical calculation which we will apply to quantum states later. It is
correct for the EM forces, but, the electron is actually in a rotating system which gives an additional
~L·S~term (not from the B field!). This term is 1/2 the size and of opposite sign. We have already
included this factor of 2 in the answer given above.
Recall that
H 2 ∝L~·~S=
1
2
[
J^2 −L^2 −S^2
]
and we will therefore want to work with states of definitej,ℓ, ands.
23.4.3 Perturbation Calculation for Relativistic Energy Shift
RewritingH 1 =−^18 p
(^4) e
m^3 c^2 asH^1 =−
1
2 mc^2
(
p^2
2 m
) 2
we calculate the energy shift for a stateψnjmjℓs.
While there is no spin involved here, we will need to use these states for the spin-orbit interaction
〈
ψnjmjℓs|H 1 |ψnjmjℓs
〉
= −
1
2 mc^2
〈
ψnjmjℓs
∣
∣
∣
∣
∣
(
p^2
2 m
) 2 ∣∣
∣
∣
∣
ψnjmjℓs
〉
= −
1
2 mc^2
〈
ψnjmjℓs
∣
∣
∣
∣
∣
(
H 0 +
e^2
r
) 2 ∣∣
∣
∣
∣
ψnjmjℓs
〉
= −
1
2 mc^2
〈
ψnjmjℓs
∣
∣
∣
∣H
2
0 +
e^2
r
H 0 +H 0
e^2
r
+
e^4
r^2
∣
∣
∣
∣ψnjmjℓs
〉
= −
1
2 mc^2
[
E^2 n+
〈
ψnjmjℓs
∣
∣
∣
∣
e^2
r
∣
∣
∣
∣H^0 ψnjmjℓs
〉
+
〈
H 0 ψnjmjℓs
∣
∣
∣
∣
e^2
r
∣
∣
∣
∣ψnjmjℓs
〉
+
〈
ψnjmjℓs
∣
∣
∣
∣
e^4
r^2
∣
∣
∣
∣ψnjmjℓs
〉]
= −
1
2 mc^2
[
E^2 n+ 2Ene^2
〈
1
r
〉
n
+e^4
〈
1
r^2
〉
nl
]
where we can use some of our previous results.
En = −
1
2
α^2 mc^2 /n^2 =
−e^2
2 a 0 n^2
〈
1
r
〉
n
=
(
1
a 0 n^2
)
〈
1
r^2
〉
=
(
1
a^20 n^3 (ℓ+^12 )
)
〈
ψnjmjℓs|H 1 |ψnjmjℓs
〉
= −
1
2 mc^2
[(
−^12 α^2 mc^2
n^2
) 2
+ 2
(
−^12 α^2 mc^2
n^2
)
e^2
a 0 n^2
+
e^4
a^20 n^3 (ℓ+^12 )
]
= −
1
2 mc^2
En(0)
2
[
1 −4 +
4 n
ℓ+^12
]
= +
En(0)
2
2 mc^2
[
3 −
4 n
ℓ+^12