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9780198538660

Radiation Trapping in Atomic Vapours

by ;
  • ISBN13:

    9780198538660

  • ISBN10:

    0198538669

  • Format: Hardcover
  • Copyright: 1999-02-25
  • Publisher: Clarendon Press

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Summary

Radiation from spectral lines can be absorbed and re- emitted many times in atomic vapours before it reaches the boundaries of the container encasing the vapour. This effect is known as radiation trapping. It plays an important role practically everywhere where atomic vapours occur, e.g. inspectroscopy, in gas lasers, in atomic line filters, in the determination of atomic lifetimes, in measurements of atomic interaction potentials, and in electric discharge lamps. This book for the first time assembles all the information necessary for a treatment of practical problems, emphasizingboth physical insights and mathematical methods. After an introduction that reviews resonance radiation and collisional processes in atomic vapours, physical effects and mathematical methods for various types of problems (e.g. with or without saturation, particle diffusion, reflecting cell walls,etc.) are explained in detail. The last part of the book describes the applications of these methods to a variety of practical problems like cross-section measurements or the design of discharge lamps.

Table of Contents

List of Symbols
ixx
I BACKGROUND
Introduction
3(12)
The physical process of radiation trapping
3(3)
Historical overview
6(3)
Applications of radiation trapping
9(3)
Outline of the book
12(3)
Atomic Lineshapes
15(18)
The Einstein theory of radiation
15(5)
Broadening mechanisms
20(10)
Natural broadening
20(1)
Doppler broadening
20(2)
Pressure broadening
22(2)
Voigt lineshapes
24(6)
Strength rules for fine and hyperfine splitting
30(3)
Collisions, quenching, and particle diffusion
33(16)
Collisional cross-sections
33(2)
Collisions between atoms of the same kind
35(1)
Collisions between atoms of different kinds
35(1)
Collisions with electrons; ionization and recombination
36(1)
Particle diffusion
37(4)
Hyperfine-structure intermixing
41(1)
Fine-structure intermixing
42(7)
II THE CLASSICAL RADIATION TRAPPING PROBLEM
Formulation of the classical problem
49(30)
The Milne equation
50(1)
The Holstein equation
51(13)
Derivation of the Holstein equation
51(5)
Idealized geometries
56(3)
Simplifying assumptions in the derivation of the Holstein equation
59(5)
The multiple-scattering representation
64(3)
The equation of radiative transfer
67(12)
The escape factor
69(10)
Mathematical methods for the Holstein equation
79(15)
The variational technique
79(7)
Exact solutions in the high-opacity case
86(3)
Van Trigt's solution
86(1)
The geometrical quantization technique
87(1)
The Fourier transform technique
88(1)
The piecewise-constant approximation
89(2)
The propagator function method
91(1)
Other computation methods
92(2)
Methods for the multiple-scattering representation
94(9)
Monte Carlo simulations
94(6)
Analytical solutions
100(3)
Fitting equations and physical interpretation
103(25)
Doppler and Lorentz lines
103(8)
Voigt lines
111(2)
Hyperfine split lines
113(5)
Higher-order modes
118(2)
Steady-state solutions of the Holstein equation
120(4)
The emergent spectrum
124(4)
The Milne and Eddington approximations
128(12)
The original Milne theory
128(3)
The angle approximation
131(3)
The generalized Eddington approximation
134(2)
The frequency approximation
136(4)
Mathematical methods for the transfer equation
140(25)
Discrete ordinate solution
140(2)
The Feautrier technique
142(7)
The basic Feautrier technique
143(5)
Modified finite-differencing equations
148(1)
Choice of the boundary conditions
149(1)
The variable Eddington factor technique
149(5)
Modified Feautrier approaches
154(11)
The Rybicki reorganization
154(2)
The core saturation method
156(1)
The implicit integral method
157(1)
Splitting algorithms
157(1)
Quadrature perturbation
158(1)
The discontinuous finite-element (DFE) method
158(7)
III GENERALIZED TRAPPING PROBLEMS
Simple generalizations
165(39)
Branching and quenching
165(2)
Three-level atoms
167(4)
Reflecting walls
171(8)
Diffusely reflecting walls
171(2)
Specularly reflecting walls
173(6)
Particle diffusion
179(14)
Formulation and direct solution
179(2)
The modal combination technique
181(5)
The discrete-ordinate technique
186(6)
Results
192(1)
Inhomogeneous distribution of absorbers
193(4)
Two- and three-dimensional geometries
197(7)
The finite cylinder
197(4)
The parallelepiped
201(1)
The torus and the hollow cylinder
201(3)
Partial frequency redistribution
204(43)
The physical picture of PFR
204(19)
Redistribution functions in the atomic rest frame
205(3)
Redistribution functions in the laboratory rest frame
208(2)
Angle-averaged redistribution functions
210(1)
Pure Doppler broadening
211(3)
Doppler plus natural broadening
214(4)
Doppler plus collisional broadening
218(1)
Doppler, natural, plus collisional broadening
219(1)
Branching transitions
220(1)
The Holstein equation with PFR
221(2)
Variational solution
223(7)
The velocity distribution of excited atoms
230(2)
The propagator function method and the PCA method
232(4)
Monte Carlo simulations
236(2)
Transfer equation formulations
238(2)
Frequency diffusion
240(2)
Large-scale particle flow
242(5)
Polarization
247(15)
Introduction
247(1)
Formal solution of the vector transfer equation
248(2)
Trapping problems with polarization
250(4)
The polarization-free approximation
250(1)
The Holstein equation without magnetic field
251(2)
The Holstein equation with magnetic field
253(1)
Monte Carlo simulations
254(4)
Physical effects
258(4)
Non-linear radiation trapping
262(51)
When do non-linearities occur?
263(4)
Interaction of strong laser radiation with atoms
267(4)
Selection of velocity groups
268(2)
Burn-through and one-dimensionality
270(1)
Steady-state solutions
271(17)
Complete linearization
272(4)
Operator perturbation
276(9)
Direct iteration
285(2)
Approximate techniques
287(1)
Monte Carlo simulations
287(1)
Transient problems
288(11)
Numerical solution of the non-linear Holstein equation
288(3)
Analytical approximations
291(2)
Numerical solution of the transfer equation
293(1)
Physical effects
294(4)
Monte Carlo simulations
298(1)
Multilevel systems
299(14)
Complete linearization in the multilevel case
299(1)
Operator perturbation techniques for multilevel systems
300(1)
The equivalent two-level atom
301(2)
Steady-state in three-level atoms
303(4)
Time-dependent depletion
307(6)
Combination of techniques
313(13)
The four basic questions
313(1)
Linear trapping with complete frequency redistribution
314(5)
Solution methods for the classical Holstein equation
314(3)
Inclusion of other physical effects
317(2)
Nonlinear trapping with CFR
319(2)
Taking the non-linearity into account
320(1)
Multilevel atoms
320(1)
Required accuracy
321(1)
Trapping with partial frequency redistribution
321(5)
IV APPLICATIONS
Measurements in chemical physics
326(20)
Atomic lifetimes
327(1)
Collision cross-sections
328(3)
Ionization cross-sections
331(4)
Quenching and intermixing cross-sections
335(3)
Atomic beams
338(1)
Atomic densities
339(1)
Radiation trapping in cold atoms
340(4)
Other measurements
344(2)
Simulation of optically pumped gas lasers
346(15)
Trapping in gas lasers
346(1)
Low-opacity formulation
347(7)
Basic formulation
347(3)
Approximate solution for single-mode operation
350(2)
Conclusions
352(2)
The mercury-nitrogen laser
354(7)
The operating principle
354(1)
Setup of the rate equations
355(3)
Conclusions
358(3)
Atomic line filters
361(7)
Discharge lamps and plasmas
368(19)
Introduction
368(1)
The theory of discharge lamps
369(3)
Radiation trapping in discharge lamps
372(4)
Decreasing radiation trapping in lamps
376(3)
The optogalvanic effect
379(2)
Plasmas
381(2)
Concluding remarks
383(4)
V APPENDICES
Atomic structure
387(16)
Models of the atomic structure
387(1)
The Bohr-Rutherford model
387(1)
The Schruodinger equation
388(1)
The hydrogen atom
388(3)
The periodic table of elements
391(1)
Alkali atoms
392(5)
Lifting of the l-degeneracy in alkali atoms
392(2)
Fine structure of alkali atoms
394(3)
The helium atom
397(2)
The alkaline earth elements
399(1)
Trivalent elements
399(1)
Hyperfine structure and isotope splitting
399(2)
Hyperfine structure
399(2)
Isotope splitting
401(1)
Effects of external magnetic and electric fields
401(2)
The Zeeman effect
401(1)
The Stark effect
402(1)
Values of the Ak.m matrix elements for the numerical solution of the Holstein equation
403(10)
The slab
403(1)
The cylinder---method 1
404(2)
The cylinder---method 2
406(3)
The sphere
409(4)
Publicly available software for the computation of radiation trapping
413(9)
Rad-Trap
413(2)
McTrap
415(3)
Slab3
418(1)
Altair
419(1)
Tlusty
420(1)
Other programs
421(1)
Fitting equations for the eigenvalues and eigenfunctions of the Holstein equation
422(5)
The slab
422(1)
The cylinder
422(1)
The sphere
423(4)
Finite difference solution of the inhomogeneous equation of radiative transfer in a finite cylinder
427(6)
The density matrix
433(7)
The density matrix for atomic states
433(1)
The density matrix for photons
434(2)
Interaction of atoms and radiation
436(1)
State multipoles
437(3)
Definition of tensor operators
437(1)
Definition of state multipoles
438(2)
High-field effects
440(6)
Absorption and emission coefficients of homogeneously broadened lines
440(1)
AC-Stark splitting and Mollow triplets
441(2)
Effects of AC-Stark splitting on radiation trapping
443(1)
The validity of the transfer equation
444(2)
References 446(55)
Index 501

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