Published January 2003
| Version v1
Journal article
Investigation of fusion yield from exploding deuterium-cluster plasmas produced by 100-TW laser pulses
Creators
- 1. Department of Physics, The University of Texas at Austin, Austin, Texas 78712 (United States)
- 2. Physics and Advanced Technology Directorate, Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
- 3. Department of Nuclear Engineering, University of California at Berkeley, Berkeley, California 94720 (United States)
Description
When clusters of deuterium are irradiated with an intense, ultrafast laser pulse, the clusters explode, generating ions with kinetic energies high enough to produce nuclear-fusion events. Here we present experimental measurements of the dependence of the fusion yield of an exploding deuterium-cluster plasma on pulse energy up to the 10-J level for incident pulse durations of 100 fs and 1 ps. These energies correspond to peak vacuum intensities of 2x1020 and 2x1019 W/cm2, respectively. We also present measurements of the resulting plasma ion spectra that possess features indicative of a Coulomb explosion and discuss the yield scaling and its relation to previous findings based on the differences in laser focal geometry and pulse duration
Additional details
Publishing Information
- Journal Title
- Journal of the Optical Society of America. Part B, Optical Physics
- Journal Volume
- 20
- Journal Issue
- 1
- Journal Page Range
- p. 113-117
- ISSN
- 0740-3224
- CODEN
- JOBPDE
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35071922
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ATOMIC CLUSTERS; DEUTERIUM; FUSION YIELD; GEOMETRY; KINETIC ENERGY; LASERS; PLASMA DIAGNOSTICS; PULSES
- Descriptors DEC
- ENERGY; HYDROGEN ISOTOPES; ISOTOPES; LIGHT NUCLEI; MATHEMATICS; NUCLEAR REACTION YIELD; NUCLEI; ODD-ODD NUCLEI; STABLE ISOTOPES; YIELDS
Optional Information
- Notes
- (c) 2003 Optical Society of America