Kinetically balanced Gaussian basis-set approach to relativistic Compton profiles of atoms
Creators
- 1. Physics Department, Indian Institute of Technology, Powai, Mumbai 400076 (India)
Description
Atomic Compton profiles (CPs) are a very important property which provide us information about the momentum distribution of atomic electrons. Therefore, for CPs of heavy atoms, relativistic effects are expected to be important, warranting a relativistic treatment of the problem. In this paper, we present an efficient approach aimed at ab initio calculations of atomic CPs within a Dirac-Hartree-Fock (DHF) formalism, employing kinetically balanced Gaussian basis functions. The approach is used to compute the CPs of noble gases ranging from He to Rn, and the results have been compared to the experimental and other theoretical data, wherever possible. The influence of the quality of the basis set on the calculated CPs has also been systematically investigated
Additional details
Identifiers
- DOI
- 10.1103/PhysRevA.75.022504;
- arXiv
- arXiv:physics/0703205v1;
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 75
- Journal Issue
- 2
- Journal Page Range
- p. 022504-022504.12
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39010854
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ATOMS; COMPTON EFFECT; COMPUTER CALCULATIONS; DIRAC EQUATION; DISTRIBUTION; ELECTRONS; GAUSSIAN PROCESSES; HARTREE-FOCK METHOD; PHOTON-ATOM COLLISIONS; RARE GASES; RELATIVISTIC RANGE
- Descriptors DEC
- APPROXIMATIONS; ATOM COLLISIONS; BASIC INTERACTIONS; CALCULATION METHODS; COLLISIONS; DIFFERENTIAL EQUATIONS; ELASTIC SCATTERING; ELECTROMAGNETIC INTERACTIONS; ELEMENTARY PARTICLES; ELEMENTS; ENERGY RANGE; EQUATIONS; FERMIONS; FIELD EQUATIONS; FLUIDS; GASES; INTERACTIONS; LEPTONS; NONMETALS; PARTIAL DIFFERENTIAL EQUATIONS; PHOTON COLLISIONS; SCATTERING; WAVE EQUATIONS
Optional Information
- Notes
- (c) 2007 The American Physical Society