Influence of gas pressure on high-order-harmonic generation of Ar and Ne
Creators
- 1. Key Laboratory of Atomic and Molecular Physics and Functional Materials of Gansu Province, College of Physics and Electronic Engineering, Northwest Normal University, Lanzhou,730070 (China)
- 2. Physics Department, J. R. Macdonald Laboratory, Kansas State University, Manhattan, Kansas 66506-2604 (United States)
Description
We study the effect of gas pressure on the generation of high-order harmonics where harmonics due to individual atoms are calculated using the recently developed quantitative rescattering theory, and the propagation of the laser and harmonics in the medium is calculated by solving the Maxwell's wave equation. We illustrate that the simulated spectra are very sensitive to the laser focusing conditions at high laser intensity and high pressure since the fundamental laser field is severely reshaped during the propagation. By comparing the simulated results with several experiments we show that the pressure dependence can be qualitatively explained. The lack of quantitative agreement is tentatively attributed to the failure of the complete knowledge of the experimental conditions.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevA.84.053404;
- arXiv
- arXiv:1107.6018v1;
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 84
- Journal Issue
- 5
- Journal Page Range
- p. 053404-053404.9
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44051957
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ATOMS; COMPUTERIZED SIMULATION; HARMONIC GENERATION; HARMONICS; LASER RADIATION; MAXWELL EQUATIONS; PRESSURE DEPENDENCE; RESCATTERING; WAVE EQUATIONS
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; ELECTROMAGNETIC RADIATION; EQUATIONS; FREQUENCY MIXING; OSCILLATIONS; PARTIAL DIFFERENTIAL EQUATIONS; RADIATIONS; SCATTERING; SIMULATION
Optional Information
- Notes
- (c) 2011 American Institute of Physics