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QM in 3D Quantum Ch.4, Physical Systems, 24.Feb.2003 EJZ. Schr ö dinger eqn in spherical coordinates Separation of variables (Prob.4.2 p.124) Angular equation (Prob.4.3 p.128 or 4.23 p.153) Hydrogen atom (Prob 4.10 p.140) Angular Momentum (Prob 4.20 p.150) Spin.
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Schrödinger eqn in spherical coordinates
Separation of variables (Prob.4.2 p.124)
Angular equation (Prob.4.3 p.128 or 4.23 p.153)
Hydrogen atom (Prob 4.10 p.140)
Angular Momentum (Prob 4.20 p.150)
The time-dependent SE in 3D
has solutions of form
where Yn(r,t) solves
Recall how to solve this using separation of variables…
Then the 3D diffeq becomes two diffeqs (one 1D, one 2D)
Let Y(q,f) = Q(q)F(f) and separate variables:
The f equation has solutions F(f) = eimf (by inspection)
and the q equation has solutions Q(q) = C Plm(cosq) where Plm = associated Legendre functions of argument (cosq).
The angular solution = spherical harmonics:
Y(q,f)= C Plm(cosq) eimfwhere C = normalization constant
In solving the angular equation, we use the Rodrigues formula to generate the Legendre functions:
“Notice that l must be a non-negative integer for [this] to make any sense; moreover, if |m|>l, then this says that Plm=0. For any given l, then there are (2l+1) possible values of m:”
Radial equation solutions for V= Coulomb potential depend on n and l(L=Laguerre polynomials, a = Bohr radius)
Angular solutions = Spherical harmonics
As we showed earlier, Energy = Bohr energy with n’=n+l.
Radial wavefunctions depend on n and l, where l = 0, 1, 2, …, n-1
Angular wavefunctions depend on l and m, where m= -l, …, 0, …, +l
Quantization of angular momentum direction for l=2
Magnetic field splits l level in (2l+1) values of ml = 0, ±1, ± 2, … ±l
L = r x p
Calculate Lx, Ly, Lz and their commutators:
Each component does commute with L2:
l = orbital quantum number
ml = magnetic quantum number = 0, ±1, ±2, …, ±l
ms = spin = ±1/2
Total angular momentum J=L+s
with j=l+s, l+s-1, …, |l-s|
Commutation relations are just like those for L:
Can measure S and Sz simultaneously, but not Sx and Sy.
Spinors = spin eigenvectors
An electron (for example) can have spin up or spin down
Next time, operate on these with Pauli spin matrices…
Multi-electron atoms have total J = S+L where
S = vector sum of spins,
L = vector sum of angular momenta
Allowed transitions (emitting or absorbing a photon of spin 1)
ΔJ = 0, ±1 (not J=0 to J=0) ΔL = 0, ±1 ΔS = 0
Δmj =0, ±1 (not 0 to 0 if ΔJ=0)
Δl = ±1 because transition emits or absorbs a photon of spin=1
Δml = 0, ±1 derived from wavefunctions and raising/lowering ops
Stern Gerlach measures me = 2 mB:
Dirac’s QM prediction = 2*Bohr’s semi-classical prediction
Zeeman effect is due to an external magnetic field.
Fine-structure splitting is due to spin-orbit coupling (and a small relativistic correction).
Hyperfine splitting is due to interaction of melectron with mproton.
Very strong external B, or “normal” Zeeman effect, decouples L and S, so geff=mL+2mS.