Published September 2004
| Version v1
Journal article
The search for dark matter via gamma rays from astronomical sources using EGRET and GLAST
Creators
- 1. Stanford Linear Accelerator Center, Stanford University 2575 Sand Hill Road, Menlo Park, CA 94025 (United States)
Description
EGRET, aboard NASA's CGRO satellite, has made important contributions to establishing limits on WIMP dark matter in the galaxy. This paper will review these EGRET results. Based on past limits and theoretical estimates, future potential dark matter results from GLAST are projected
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2004.08.016;
- PII
- S0920-5632(04)00306-8;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 134
- Journal Issue
- 3
- Journal Page Range
- p. 103-111
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 2. international conference on particle and fundamental physics in space
- Acronym
- SpacePart '03
- Dates
- 10-12 Dec 2003
- Place
- Washington, DC (United States)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36051474
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC PHOTONS; COSMIC RAY DETECTION; GALAXIES; GAMMA RADIATION; NONLUMINOUS MATTER; PARTICLE IDENTIFICATION; SATELLITES; WEAK INTERACTIONS
- Descriptors DEC
- BASIC INTERACTIONS; BOSONS; COSMIC RADIATION; DETECTION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; INTERACTIONS; IONIZING RADIATIONS; MASSLESS PARTICLES; MATTER; PHOTONS; RADIATION DETECTION; RADIATIONS
Optional Information
- Copyright
- Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.