Published October 2012
| Version v1
Journal article
The photonuclear neutron and gamma-ray backgrounds in the fast ignition experiment
Creators
- 1. Institute of Laser Engineering, Osaka University, 2-6 Yamadaoka Suita (Japan)
- 2. National Institution Fusion Science, 322-6 Oroshi-cho, Toki-city, Gifu (Japan)
Description
In the fast-ignition scheme, very hard x-rays (hereinafter referred to as γ-rays) are generated by Bremsstrahlung radiation from fast electrons. Significant backgrounds were observed around the deuterium–deuterium fusion neutron signals in the experiment in 2010. In this paper the backgrounds were studied in detail, based on Monte Carlo simulations, and they were confirmed to be γ-rays from the target, scattered γ-rays from the experimental bay walls (γ′-rays), and neutrons generated by (γ, n) reactions in either the target vacuum chamber or the diagnostic instruments (γ-n neutrons).
Additional details
Identifiers
- DOI
- 10.1063/1.4732180;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 83
- Journal Issue
- 10
- Journal Page Range
- p. 10D909-10D909.3
- ISSN
- 0034-6748
- CODEN
- RSINAK
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44052280
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- BREMSSTRAHLUNG; COMPUTERIZED SIMULATION; DEUTERIUM; GAMMA RADIATION; HARD X RADIATION; MONTE CARLO METHOD; NEUTRONS; PHOTON-NUCLEON INTERACTIONS; PHOTONUCLEAR REACTIONS; THERMONUCLEAR IGNITION; THERMONUCLEAR REACTORS
- Descriptors DEC
- BARYONS; BASIC INTERACTIONS; CALCULATION METHODS; ELECTROMAGNETIC INTERACTIONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN ISOTOPES; INTERACTIONS; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; NUCLEAR REACTIONS; NUCLEI; NUCLEONS; ODD-ODD NUCLEI; PARTICLE INTERACTIONS; PHOTON-BARYON INTERACTIONS; PHOTON-HADRON INTERACTIONS; RADIATIONS; SIMULATION; STABLE ISOTOPES; X RADIATION
Optional Information
- Notes
- (c) 2012 American Institute of Physics