QM in 3D Quantum Ch.4, Physical Systems, 24.Feb.2003 EJZ - PowerPoint PPT Presentation

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QM in 3D Quantum Ch.4, Physical Systems, 24.Feb.2003 EJZ

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... equation, we use the Rodrigues formula to generate the Legendre functions: ... Angular momentum L: from Classical physics to QM. L = r x p ... – PowerPoint PPT presentation

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Title: QM in 3D Quantum Ch.4, Physical Systems, 24.Feb.2003 EJZ


1
QM in 3DQuantum Ch.4, Physical Systems,
24.Feb.2003 EJZ
Schrödinger eqn in spherical coordinates Separatio
n 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
2
Schrödinger eqn. in spherical coords.
The time-dependent SE in 3D
has solutions of form where Yn(r,t)
solves Recall how to solve this using
separation of variables
3
Separation of variables
To solve Let Then the 3D diffeq becomes two
diffeqs (one 1D, one 2D) Radial
equation Angular equation
4
Solving the Angular equation
To solve 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) eimf where C
normalization constant
5
Quantization of l and m
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 mgtl, then this says that
Plm0. For any given l, then there are (2l1)
possible values of m (Griffiths p.127)
6
Solving the Radial equation
7
finish solving the Radial equation
8
Solutions to 3D spherical Schrödinger eqn
Radial equation solutions for V Coulomb
potential depend on n and l (LLaguerre
polynomials, a Bohr radius)
Rnl(r) Angular solutions Spherical
harmonics As we showed earlier, Energy Bohr
energy with nnl.
9
Hydrogen atom a few wave functions
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
10
Angular momentum L review from Modern physics
Quantization of angular momentum direction for
l2
Magnetic field splits l level in (2l1) values of
ml 0, 1, 2, l
11
Angular momentum L from Classical physics to QM
L r x p Calculate Lx, Ly, Lz and their
commutators Uncertainty relations Each
component does commute with L2 Eigenvalues
12
Spin - review
  • Hydrogen atom so far 3D spherical solution to
    Schrödinger equation yields 3 new quantum
    numbers
  • l orbital quantum number
  • ml magnetic quantum number 0, 1, 2, , l
  • ms spin 1/2
  • Next step toward refining the H-atom model
  • Spin with
  • Total angular momentum JLs
  • with jls, ls-1, , l-s

13
Spin - new
  • 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

14
Total angular momentum
  • Multi-electron atoms have total J SL where
  • S vector sum of spins,
  • L vector sum of angular momenta
  • Allowed transitions (emitting or absorbing a
    photon of spin 1)
  • ?J 0, 1 (not J0 to J0) ?L 0, 1
    ?S 0
  • ?mj 0, 1 (not 0 to 0 if ?J0)
  • ?l 1 because transition emits or absorbs a
    photon of spin1
  • ?ml 0, 1 derived from wavefunctions and
    raising/lowering ops

15
Review applications of Spin
  • Bohr magneton
  • Stern Gerlach measures me 2 m B
  • Diracs QM prediction 2Bohrs 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 geffmL2mS.
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