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Lecture Notes 0
Class organization.
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Lecture Notes 1
Classical physics ca.1900. CM and EM, relativity;
atomic stability; spectral lines; black body radiation, density of
states; Planck's hypothesis.
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Lecture Notes 2
"Old" quantum mechanics,
Bohr H atom;
de Broglie, pilot waves;
Davisson and Germer;
free Schrödinger equation, eigenfunctions and
eigenvalues;
full time-dependent and time-independent Schrödinger equation;
Copenhagen interpretation; constant potential; qualitative nature of
1D wavefunctions; 1D infinite square well.
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Lecture Notes 3
1D infinite square well.
Normalization.
Heisenberg Uncertainty Principle.
Finite depth 1D square well, boundary conditions on psi(x).
1D SHO, ground state and excited states.
Expectation values, SHO examples, "sandwich formula."
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QM Aside 0
Graphical solution of 1D finite square well (even) bound states. (pdf)
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QM Aside 1
Calculation of SHO matrix elements using explicit wfns. (pdf)
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QM Aside 2
Creation and annihilation (raising and lowering) operators for the 1D SHO. (pdf)
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QM Aside 3
Beautiful 1D SHO wfn plots (postscript):
psi_0
psi_1
psi_2
psi_3
psi_n, n=0,100
psi_n, n=0,100 (detail)
|psi^2| for n=0, 100
|psi^2| for n=100 versus
P_classical
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Lecture Notes 4
3D bound state problems. Schrödinger equation in spherical
coordinates. Separation of variables, Legendre functions and spherical
harmonics. Radial wavefunction and centrifugal barrier. Angular momentum
operators, their eigenvalues and commutation relations.
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Lecture Notes 5
3D Coulomb and SHO problems.
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Summary for midterm
Pre-midterm summary of topics.
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Lecture Notes 6
Nondegenerate perturbation theory: general results.
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QM Aside 4.
High order perturbation theory example: 1D SHO with H_I = gx^4.
{c_n}
E_0(g) coeffs
analytically to 33rd order! (also gives their prime factors)
plot of |c_n|, log/lin
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Lecture Notes 7
Variational method.
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Lecture Notes 8
Degenerate perturbation theory. Stark effect.
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Lecture Notes 9
Spin, general results. Interaction with magnetic fields.
Combining two spin-1/2 states.
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Lecture Notes 10
General S1xS2 Clebsch-Gordan problem.
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Gaunt formula
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Irreducible tensor operators and the
Wigner-Eckhart theorem
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Helium
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Probability current
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QM Aside 5.
Current densities in hydrogen (png):
2P(m=+1)
3D(m=+2)
3D(m=+1)
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2nd order Stark effect
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