Self-focusing, Raman, and modulation instability of shaped relativistic laser pulse in plasmas
Creators
- 1. State Key Laboratory of High Field Laser Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Science, P.O. Box 800-211, Shanghai 201800 (China)
Description
The interaction of shaped laser pulses with plasmas is studied in a strict theoretical framework without adopting the slow-varying envelope approximation (SVEA). Any physical quantities involved in the interaction are denoted as a summation of different real quantities of respective phases. The relationships among the phases of those real quantities and their moduli are strictly analyzed. Such strict analyses lead to a more exact equation set for the three-dimensional envelope of the laser pulse, which is not based on SVEA. Based on this equation set, self-focusing, Raman, and modulation instabilities could be discussed in a unified framework. The solutions of this equation set for the laser envelope reveal many possible multicolor laser modes in plasmas. The energy and the shape of a pulse determine its propagation through plasmas in a multicolor mode or in a monochromic mode. A global growth rate is introduced to measure the speed of the transition from the monochromic mode in vacuum to a possible mode in plasmas
Additional details
Identifiers
- DOI
- 10.1063/1.2357725;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 13
- Journal Issue
- 10
- Journal Page Range
- p. 103105-103105.12
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38023285
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- APPROXIMATIONS; BEAM-PLASMA SYSTEMS; LASER RADIATION; LIGHT TRANSMISSION; MODULATION; PLASMA INSTABILITY; PULSES; RELATIVISTIC PLASMA; RELATIVISTIC RANGE
- Descriptors DEC
- CALCULATION METHODS; ELECTROMAGNETIC RADIATION; ENERGY RANGE; INSTABILITY; PLASMA; RADIATIONS; TRANSMISSION
Optional Information
- Notes
- (c) 2006 American Institute of Physics