Theory of high-order harmonic generation in relativistic laser interaction with overdense plasma
Creators
- 1. Institut fuer Theoretische Physik I, Heinrich-Heine-Universitaet Duesseldorf, D-40225 Dusseldorf (Germany)
- 2. L.D. Landau Institute for Theoretical Physics, Moscow (Russian Federation)
Description
High-order harmonic generation due to the interaction of a short ultrarelativistic laser pulse with overdense plasma is studied analytically and numerically. On the basis of the ultrarelativistic similarity theory we show that the high-order harmonic spectrum is universal, i.e., it does not depend on the interaction details. The spectrum includes the power-law part In∝n-8,n∼3 for n<√(8α)γmax3, followed by exponential decay. Here γmax is the largest relativistic γ factor of the plasma surface and α is the second derivative of the surface velocity at this moment. The high-order harmonic cutoff at ∝γmax3 is parametrically larger than the 4γmax2 predicted by the simple ''oscillating mirror'' model based on the Doppler effect. The cornerstone of our theory is the new physical phenomenon: spikes in the relativistic γ factor of the plasma surface. These spikes define the high-order harmonic spectrum and lead to attosecond pulses in the reflected radiation
Additional details
Identifiers
- DOI
- 10.1103/PhysRevE.74.046404;
- arXiv
- arXiv:physics/0604228v1;
Publishing Information
- Journal Title
- Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics
- Journal Volume
- 74
- Journal Issue
- 4
- Journal Page Range
- p. 046404-046404.11
- ISSN
- 1063-651X
- CODEN
- PLEEE8
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39085697
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- BEAM-PLASMA SYSTEMS; DOPPLER EFFECT; ENERGY SPECTRA; HARMONIC GENERATION; LASERS; PLASMA DENSITY; PULSES; RELATIVISTIC PLASMA
- Descriptors DEC
- FREQUENCY MIXING; PLASMA; SPECTRA
Optional Information
- Notes
- (c) 2006 The American Physical Society