130_notes.dvi

(Frankie) #1

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

]
Free download pdf