Laser wake-field acceleration in pre-formed plasma channel created by pre-pulse pedestal of terawatt laser pulse
Creators
- 1. Laser Plasma Division, Raja Ramanna Centre for Advanced Technology, Indore 452 013 (India)
Description
The role of nanosecond duration pre-pulse pedestal (Amplified Spontaneous Emission (ASE) pre-pulse) in the propagation of 45 fs, 4 TW Ti:Sapphire laser pulse through a helium gas jet target has been investigated. We observed that the pre-pulse pedestal of about 1 ns duration and intensity 3 x 1012 W/cm2 creates pre-formed plasma with optical guiding channel like structure in the gas-jet at density around 3 x 1019 cm-3. Guiding of the 45 fs laser pulse (IL = 3 x 1018 W/cm2) in the pre-formed plasma channel, over a distance much longer than the Rayleigh length was also observed. The guiding of the laser pulse resulted in the generation of high energy electron beam by laser wake-field acceleration of self-injected electrons. The accelerated electron beam was quasi-monoenergetic with peak energy up to 50 MeV, low divergence in the range of 3-6 mrad, and bunch charge up to 100 pC.
Additional details
Identifiers
- DOI
- 10.1063/1.3629983;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 9
- Journal Page Range
- p. 093104-093104.9
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44002971
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ACCELERATION; DENSITY; ELECTRON BEAMS; EMISSION; HELIUM; LASER RADIATION; MEV RANGE 10-100; PEAKS; PLASMA; PLASMA GUNS; POWER RANGE 01-10 TW; PULSES; WAKEFIELD ACCELERATORS
- Descriptors DEC
- ACCELERATORS; BEAMS; ELECTROMAGNETIC RADIATION; ELEMENTS; ENERGY RANGE; FLUIDS; GASES; LEPTON BEAMS; LINEAR ACCELERATORS; MEV RANGE; NONMETALS; PARTICLE BEAMS; PHYSICAL PROPERTIES; POWER RANGE; RADIATIONS; RARE GASES; TERAWATT POWER RANGE
Optional Information
- Notes
- (c) 2011 American Institute of Physics