Chapter 8 - Atomic Structure and Lifetimes
Applications
Forbidden transitions
Inevitability of decay?
Multipole radiation in He-like atoms
M1 - easier than E1 (Sect. 8.1-8.2)
Models for E1 and M1 transitions
Electric and magnetic dipoles
Compare Z dependences
Line strength factors
Empirical specification
Tabulation
Fine structures
Examples
Intermediate coupling channels
IC line strengths, sp
IC line strengths, p2
M1 line strengths
Application: Si-like Kr22+
Isoelectronic application
Ordering of relativistic corrections
Astrophysical implications (Sect. 8.2)
The Solar Corona
Helium
Eclipse photo and coronium
Solar corona, before 1930
Lyot solar camera
Coronagraph spectrum
Coronium and Edlén
Bengt Edlén and King Gustaf VI Adolf,
1951
Why Edlén abandoned his thesis work
Gröna jorden?
Solar temperatures
Grotrian and Edlén
Highly ionized lab spectra
Identified lines
Compute np and np5 A's
Compute IC A's
Analysis of solar data
Temperature broadening
Doppler width
Solar temperatures
Nebulium and the O III ground configuration
Example: p3 configuration (Sect. 8.2.4)
2 nonequivalent electrons
2 equivalent electrons
3 equivalent p electrons
LS to jj
Matrix
Inversion of coefficients from known roots
Slater/spin-orbit parameters from measured energies
Application
Find vectors
Physical eigenvectors
Matrix diagonalization
Tabulation
Matrix multiplication
Line strength array
Fe 19+
P sequence
Deferred Topics
s2p and s2p5 ground configs
Reduction formula
n=2 B and F sequences
n=3 Al and Cl sequences
n=4,5,6 sequences
Ga sequence
Fits
Isoelectronic plots
Ground states
p2 and p4 ground state
configurations
M1 with intermediate coupling
Line strengths for sp
Line strengths for p2 and
p4
Kr22+: line strengths
-Transition probability
-Lifetime
Si sequence
S sequence
Formulae
p3 ground configurations
p3 levels from LS to
jj
Off-diagonal Hamiltonian
Polynomial reduction
Reduction
Application to Fe19+
Computed eigenvectors
Vectors and matrices
Matrix product
Compare with ab initio
P sequence