Chapter 2 - Atomic Structure and Lifetimes
Semiclassical Conceptual Models
Discover Magazine - Lee Smolin
Part I: Classical Position Probability Densities (Sect.2.1.1)
Announcement
Källén Prize
Gas laws
Microscopic origin of pressure
End-on dipole
Induced dipole
6-12 potential
Not really 12
van der Waals equation
Is pressure a force or an energy?
Animation I
Animation II
Molecule in a room (Sect. 2.1.2)
Probability formulation
EBK box quantization
Energy levels
Classical and BSW
Mean position
Mean square position
Measurements
Variance and standard deviation
Variance of distributions
Experimental testing
Harmonic oscillator (Sect. 2.3.3)
Generalized formulation
SHO average values
Action quantization
Classical and BSW
Summary
Anharmonic well
Perturbation expansion
Accepted QM solution
Animation
Comparison with box and Kepler
Generalize to numerical solution of arbitrary potentials
Formulation
Exercise
Solution
Semiclassical Quantization (Sect. 2.3)
BSW Quantization
EKB Quantization
EKB References
Sommerfeld and Caustics
Caustic animation
In original language
A.Einstein, Deutsche Physikalische Gesellschaft
19 (1917).
Stone essay
J.B. Keller, Ann. Phys. (NY) 4, 180 (1958).
Semiclassical self-consistent fields
Part II: The Kepler-Coulomb Potential (Sect. 2.4)
The probabilistic Kepler problem
Kepler's laws
3rd law from circular case
Virial theorem
Radial probabilities
Conservation laws
The radial derivative
Average values of powers of r (Sect. 2.4.3)
Kepler average values from radial distribution
Kepler average values from SHO solution
Kepler average values from azimuthal distribution
Laplace integral
Legendre polynomials
Classical values for rk
Classical values for rk
Quantum values for rk
Avg for powers of r
Atomic perturbations
The EKB Kepler problem (Sect. 2.4.4)
Spherical polar coordinates
Generalized momenta
Action formulation
Nonrel angle-action
Classical and QM observables
EBK ellipses and probabilities
EBK orbits, n=1,2,3
EBK orbits, n=4
Emission spectrum
Balmer series
EBK and QM radial wave functions (Sect. 2.4.5)
EBK Summary
Y(1s),
Y(2s),Y(2p)
Y(3s),
Y(3p),Y(3d)
Y(n=40,l=20)
Orbital distributions
Electron configurations
QM and classical
More QM Distributions
Morphologies
Eta Carina
More morphologies
High res
Yet another morphology
Trojan asteroids
Lagrange points
2.7 degree
BBrad
WMAP
Trojan asteroids (animation)
Wave packets of
high Rydberg states
Whole number of heartbeats per cycle
Three recent publications
Curtis & Ellis, Use of the EBK action
quantization, Am.J.Phys. 72 1521 (2004)
Curtis & Ellis, Probabilities as a Bridge
between Classical & QM Treatments, Eur.J.Phys. (in press)
Larkoski, Ellis, & Curtis, Numerical
implementation of the EBK quantization for arbitrary
potentials, Am.J.Phys. (submitted)
Part III: Applications to atoms and planets (Sect. 2.4.7)
Perturbations
Orbital precession
Mechanics and electrodynamics of moving bodies
Maxwell's equations
Invariance of the speed of light
Apparent length contraction applet
Apparent time dilation applet
Why does length contract and time dilate?
Model for magnetism
Force between a moving charge and a current
Reverse direction
Priority
Einstein, Ann. Phys. Chim. 17, 890-921 (1905).
English translation
Woldemar Voigt's 1887 discovery
Voigt bio
Relativistic corrections to the kinetic energy (Sect. 2.4.8)
Rotations among four-vectors
Space-time transformations of momentum and energy
Mass-energy: just a units conversion
Special Relativity Corrections
Magnetic moments
Torque on a current loop
Magnetic moment of an orbiting charge
Magnetic moment of a Dirac electron
Speed of an electron of finite radius
Zitterbewegung of a point charge
Zitterbewegung animation
Relativistic corrections to the potential energy (Sect. 2.4.9)
Spin-orbit fine structure
EBK and QM formulations
Foldy-Wouthuysen transformation
Gen.Rel. and Spin-Orbit
The Triplets of Belleville and Einstein
Combining relativistic corrections
Combining relativistic mass and spin-orbit
Explicit calculations for spin 1/2
Expansion of the Dirac equation
Strengths of internal fields
Thomas precession g-1, not g/2
Core polarization model (Sect. 2.4.10)
Hydrogen, hydrogenlike, and Rydberg atoms
Nonpenetrating orbits
EBK formulation of polarization
Multipole expansion
The two-center problem
Dipole moments
Multipoles in external fields
Quadrupole moments
EKB expectation values
Na-like P IV example
Schrödinger expectation values
The quantum defect parametrization
Expansion of Rydberg's formula
n-dependence of powers of r
Planetary perturbations (Sect. 2.4.11)
Potential due to a ring
Perturbations of the Planets
Masses and orbital data
Average powers of r
Effects on the period of Mercury
Test of relativity
Part IV: Self-Consistent Fields for Many-Electron Atoms (Sect. 2.4.12)
Point nucleus with homogeneous electron cloud
Potential energy with screening
Internal and external screening
1-D radial probability distribution
Semimajor axes from energies
Semiclassical Self Consistent Field Calculations
EBK for the Many-Body Problem
Newton-Raphson method
Y(QM) and
Y(EBK)
Comparison with HF for Na seq
Relativistic Semiempirical Formulation (Sect. 2.4.13)
Artifact in Cu seq
Relativistic radial momentum
Convert to atomic units
Turning points
Relativistic EBK quantization
Expansion of relativistic energy
Collapse of the Maslov Perihelion
Calculated examples of turning points
Part V: Time Dependent Processes (Sect. 2.5)
Larmor's formula
Maxwell Radiation
Classical vs QM
Wien's model (Sect. 2.5.1)
Wien model
Correspondence limit
Compare to QM
Large n limit
Worst case value
Wien's paper (1)
Wien's paper (2)
Wien's paper (3)
Comparison
Blending
Branched decay
Oscillator strength (Sect. 2.5.2)
Merzbacher's QM book
Blade article
Physics Letters article
Lorentz-Drude model
Express as oscillators
Oscillator strength
Relationships between absorption and emission
Kleppner essay