Dark Matter Searches
Creators
- 1. Kamioka Observatory, Institute for the Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka-cho, Hida-city, Gifu-prefecture (Japan)
Description
Recent cosmological as well as historical observations of rotational curves of galaxies strongly suggest the existence of dark matter. It is also widely believed that dark matter consists of unknown elementary particles. However, astrophysical observations based on gravitational effects alone do not provide sufficient information on the properties of dark matter. In this study, the status of dark matter searches is investigated by observing high-energy neutrinos from the sun and the earth and by observing nuclear recoils in laboratory targets. The successful detection of dark matter by these methods facilitates systematic studies of its properties. Finally, the XMASS experiment, which is due to start at the Kamioka Observatory, is introduced
Additional details
Identifiers
- DOI
- 10.1063/1.2899007;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 981
- Journal Issue
- 1
- Journal Page Range
- p. 80-83
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 9. international workshop on neutrino factories, superbeams and beta beams
- Acronym
- NuFact 07
- Dates
- 6-11 Aug 2007
- Place
- Okayama (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39072385
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMIC NEUTRINOS; COSMOLOGY; NEUTRINO REACTIONS; NONLUMINOUS MATTER; PARTICLE IDENTIFICATION; RECOILS; SOLID SCINTILLATION DETECTORS
- Descriptors DEC
- COSMIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTON REACTIONS; LEPTONS; MASSLESS PARTICLES; MATTER; MEASURING INSTRUMENTS; NEUTRINOS; NUCLEAR REACTIONS; PHYSICS; RADIATION DETECTORS; RADIATIONS; SCINTILLATION COUNTERS
Optional Information
- Notes
- (c) 2008 American Institute of Physics