Published November 18, 2002
| Version v1
Journal article
Characteristics of relativistic nonlinear Thomson scattering of an intense laser field as ultrashort x-ray source
- 1. Laboratory for Quantum Optics, Korea Atomic Energy Research Institute, P. O. Box 105, Deokjin-Dong, Yuseong-Ku, Daejeon, 305-600 (Korea, Republic of)
- 2. Physics Department, Pohang Univ. of Science and Technology, San 31, Hyoja-Dong, Nam-Ku, Pohang, 790-784 (Korea, Republic of)
Description
Radiations from a single electron irradiated by an ultra-intense laser pulse were extensively investigated by a numerical simulation. The characteristics of the radiation such as spectral distribution, radiation intensity, and angular distribution show that the relativistic nonlinear Thomson scattering, or Larmor radiation could be a good ultrashort radiation source toward x-ray region. The effect of ions which generates Bremsstrahlung radiation degrading the characteristics of Larmor radiation is also discussed
Additional details
Identifiers
- DOI
- 10.1063/1.1521046;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 641
- Journal Issue
- 1
- Journal Page Range
- p. 373-378
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 8. international conference on X-ray lasers
- Dates
- 27-31 May 2002
- Place
- Aspen, CO (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35090925
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANGULAR DISTRIBUTION; BREMSSTRAHLUNG; ELECTRON BEAMS; PULSE GENERATORS; RELATIVISTIC RANGE; SIMULATION; THOMSON SCATTERING; X-RAY LASERS; X-RAY SOURCES
- Descriptors DEC
- BEAMS; DISTRIBUTION; ELECTROMAGNETIC RADIATION; ELECTRONIC EQUIPMENT; ENERGY RANGE; EQUIPMENT; FUNCTION GENERATORS; INELASTIC SCATTERING; LASERS; LEPTON BEAMS; PARTICLE BEAMS; RADIATION SOURCES; RADIATIONS; SCATTERING
Optional Information
- Notes
- (c) 2002 American Institute of Physics