Extended theory of Kapitza-Dirac scattering
Creators
- 1. Department of Physics, New York University, New York, New York 10003 (United States)
Description
The standard theoretical treatment of the Kapitza-Dirac effect--that is, the scattering of an electron passing through a standing-wave laser field--is extended here through the use of the Pauli equation to account for the interaction of the electron spin with the magnetic field of the standing wave. Prescriptions for determining unitarity-preserving approximations for the transition probabilities for scattering both with and without rotation of the electron spin direction are provided. This formalism is used to develop a perturbation theory for the spin-flip probability which, in the strong-field limit of interest here, reduces to a fairly simple relation between S-matrix elements for scattering with and without change in spin orientation, each expressed in terms of a Bessel function. A similar perturbative procedure is applied to estimate corrections to the standard theory for scattering in the absence of spin-flip processes, in which interactions that change the net number of photons in the field are ignored
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 70
- Journal Issue
- 2
- Journal Page Range
- p. 023401-023401.6
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36086906
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ALGEBRA; BESSEL FUNCTIONS; CORRECTIONS; ELECTRONS; LASER RADIATION; MAGNETIC FIELDS; OPTICS; PERTURBATION THEORY; PHOTONS; PROBABILITY; QUANTUM MECHANICS; ROTATION; S MATRIX; SCATTERING; SPIN; SPIN FLIP; SPIN ORIENTATION; STANDING WAVES; UNITARITY
- Descriptors DEC
- ANGULAR MOMENTUM; BOSONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; FUNCTIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICS; MATRICES; MECHANICS; MOTION; ORIENTATION; PARTICLE PROPERTIES; RADIATIONS
Optional Information
- Notes
- (c) 2004 The American Physical Society