Published April 22, 2002
| Version v1
Journal article
Table-top neutron source for characterization and calibration of dark matter detectors
Creators
- 1. Dark Matter Group, Blackett Laboratory, Imperial College, London SW7 2BZ (United Kingdom)
- 2. Plasma Physics Group, Blackett Laboratory, Imperial College, London SW7 2BZ (United Kingdom)
Description
A table-top plasma focus device is shown to be an ideal neutron source for the calibration and characterization of dark matter detectors and has been optimized to produce a maximum yield of 2.0x107 neutrons per shot. The interaction of energetic neutrons is similar to that expected from weakly interacting massive particles (WIMPs) - a favored candidate for the dominant component of dark matter in the universe. The weak interaction of a neutron with liquid xenon gas was measured in a prototype xenon two-phase detector. We have developed a detector system in which both the primary scintillation and ionization from the initial interaction can be detected. Both measurements are critical for identifying WIMP's
Additional details
Identifiers
- DOI
- 10.1063/1.1469217;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 80
- Journal Issue
- 16
- Journal Page Range
- p. 3009-3011
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35002115
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- CALIBRATION; COSMIC RAY DETECTION; GAS SCINTILLATION DETECTORS; IONIZATION CHAMBERS; NEUTRON SOURCES; NONLUMINOUS MATTER; PLASMA FOCUS; PLASTIC SCINTILLATION DETECTORS; WEAK INTERACTIONS; XENON
- Descriptors DEC
- BASIC INTERACTIONS; DETECTION; ELEMENTS; FLUIDS; GASES; INTERACTIONS; MATTER; MEASURING INSTRUMENTS; NONMETALS; PARTICLE SOURCES; RADIATION DETECTION; RADIATION DETECTORS; RADIATION SOURCES; RARE GASES; SCINTILLATION COUNTERS; SOLID SCINTILLATION DETECTORS
Optional Information
- Notes
- (c) 2002 American Institute of Physics.