Sub-structure of laser generated harmonics reveals plasma dynamics of a relativistically oscillating mirror
Creators
- 1. Max-Born-Institut für Nichtlineare Optik und Kurzzeitspektroskopie, Max Born Str. 2A, 12489 Berlin (Germany)
- 2. Vavilov State Optical Institute, Birzhevaya line 4, 199034 St. Petersburg (Russian Federation)
Description
Theoretical and experimental investigations of the dynamics of a relativistically oscillating plasma slab reveal spectral line splitting in laser driven harmonic spectra, leading to double harmonic series. Both series are well characterized with harmonics arising by two fundamental frequencies. While a relativistic oscillation of the critical density drives the harmonic emission, the splitting is a result of an additional acceleration during the laser pulse duration. In comparison with the oscillatory movement, this acceleration is rather weak and can be described by a plasma shock wave driven by the pressure of light. We introduce particle in cell simulations and an analytical model explaining the harmonic line splitting. The derived analytical formula gives direct access between the splitting in the harmonic spectrum and the acceleration of the plasma surface
Additional details
Identifiers
- DOI
- 10.1063/1.4817807;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 20
- Journal Issue
- 8
- Journal Page Range
- p. 083109-083109.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45041622
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ACCELERATION; COMPARATIVE EVALUATIONS; EMISSION; HARMONICS; LASERS; LIGHT TRANSMISSION; MIRRORS; PLASMA DENSITY; PLASMA SIMULATION; PLASMA WAVES; RELATIVISTIC PLASMA; RELATIVISTIC RANGE; SHOCK WAVES; SPECTRA
- Descriptors DEC
- ENERGY RANGE; EVALUATION; OSCILLATIONS; PLASMA; SIMULATION; TRANSMISSION
Optional Information
- Notes
- (c) 2013 AIP Publishing LLC