Published December 2010 | Version v1
Journal article

Strong-field ionization of a heteronuclear diatomic molecule

  • 1. Institute of Advanced Energy, Kyoto University, Gokasho, Uji, Kyoto 611-0011 (Japan)

Description

We theoretically study strong-field ionization of a heteronuclear diatomic molecule, CO, by calculating the photoelectron angular distributions (PADs) and the total ionization rates using linearly and circularly polarized laser fields. We find that, although the PADs of CO generally do not have inversion symmetry, they become more inversion symmetric as the photoelectron energy increases. Heteronuclear features of CO upon ionization are better understood by comparing the results with those of a representative of homonuclear molecules, N2, in that, although there are some similarities between CO and N2 due to the same orbital symmetry, σg, there are some differences between them in terms of the ionization suppression and orientation dependence of the total ionization yield. Namely, CO behaves more like an atom in the low-intensity range in a sense that ionization takes place mainly from the neighborhood of the C core, while it behaves more like a double-core molecule in the high-intensity range since ionization takes place from the neighborhood of both C and O cores. This explains why ionization suppression of CO is not seen at the low intensity but it becomes more visible at the high intensity range.

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. A
Journal Volume
82
Journal Issue
6
Journal Page Range
p. 063410-063410.8
ISSN
1050-2947
CODEN
PLRAAN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43008747
Subject category
S74: ATOMIC AND MOLECULAR PHYSICS;
Descriptors DEI
ANGULAR DISTRIBUTION; ATOMS; CARBON MONOXIDE; IONIZATION; LASER RADIATION; MOLECULES; SYMMETRY
Descriptors DEC
CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; DISTRIBUTION; ELECTROMAGNETIC RADIATION; OXIDES; OXYGEN COMPOUNDS; RADIATIONS

Optional Information

Notes
(c) 2010 The American Physical Society