Published April 2007
| Version v1
Journal article
Searching sterile dark matter with x-ray telescopes
Creators
- 1. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547 (United States)
Description
Sterile neutrinos with masses in the keV range can be the cosmological dark matter, and they can also solve several other astrophysical puzzles. In particular, the anisotropic emission of sterile neutrinos from a supernova can explain the observed velocities of pulsars. The x-ray photons from the decays of the relic sterile neutrinos could have ionized the primordial gas, speeding up the molecular hydrogen production and, ultimately, the star formation. Precision x-ray spectroscopy can be used to search for this form of dark matter
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2006.12.068;
- PII
- S0920-5632(06)00998-4;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 166
- Journal Page Range
- p. 50-55
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 3. international conference on particle and fundamental physics in space
- Dates
- 19-21 Apr 2006
- Place
- Beijing (China)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39078410
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANISOTROPY; ASTROPHYSICS; EMISSION; HYDROGEN PRODUCTION; KEV RANGE; MASS; NEUTRINOS; NONLUMINOUS MATTER; PARTICLE DECAY; PHOTONS; PULSARS; SUPERNOVAE; TELESCOPES; X RADIATION; X-RAY DETECTION; X-RAY SPECTROSCOPY
- Descriptors DEC
- BINARY STARS; BOSONS; COSMIC RADIO SOURCES; DECAY; DETECTION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY RANGE; ERUPTIVE VARIABLE STARS; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; PHYSICS; RADIATION DETECTION; RADIATIONS; SPECTROSCOPY; STARS; VARIABLE STARS
Optional Information
- Copyright
- Copyright (c) 2007 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.