Published May 28, 2010
| Version v1
Journal article
Intense High-Contrast Femtosecond K-Shell X-Ray Source from Laser-Driven Ar Clusters
Creators
- 1. Beijing National Laboratory of Condensed Matter Physics, Institute of Physics, CAS, Beijing 100080 (China)
- 2. Advanced Photon Research Center, Japan Atomic Energy Agency, 8-1 Umemidai Kizugawa, Kyoto 619-0215 (Japan)
- 3. Department of Physics, Shanghai Jiao Tong University, Shanghai 200240 (China)
Description
Bright Ar quasimonochromatic K-shell x ray with very little background has been generated using an Ar clustering gas jet target irradiated with a 30 fs ultrahigh-contrast laser, with a measured flux of 2.2x1011 photons/J into 4π. This intense x-ray source critically depends on the laser contrast and intensity. The optimization of source output with interaction length is addressed. Simulations point to a nonlinear resonant mechanism of electron heating during the early stage of laser interaction, resulting in enhanced x-ray emission. The x-ray pulse duration is expected to be only 10 fs, opening the possibility for single-shot ultrafast keV x-ray imaging applications.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.104.215004;
- arXiv
- arXiv:0907.3421v1;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 104
- Journal Issue
- 21
- Journal Page Range
- p. 215004-215004.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42003866
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ARGON; ATOMIC CLUSTERS; ELECTRONS; FLUX DENSITY; K SHELL; KEV RANGE; LASERS; OPTIMIZATION; PHOTONS; PULSES; RESONANCE; X-RAY EMISSION ANALYSIS; X-RAY SOURCES
- Descriptors DEC
- BOSONS; CHEMICAL ANALYSIS; ELECTRONIC STRUCTURE; ELEMENTARY PARTICLES; ELEMENTS; ENERGY RANGE; FERMIONS; FLUIDS; GASES; LEPTONS; MASSLESS PARTICLES; NONDESTRUCTIVE ANALYSIS; NONMETALS; RADIATION SOURCES; RARE GASES
Optional Information
- Notes
- (c) 2010 The American Physical Society