Published 1983
| Version v1
Journal article
e+-e- annihilation and the Cosmic X-ray Background
Description
The possibility that the processes responsible for the Cosmic X-ray Background (CXB) would also produce an e--e+ annihilation feature is examined. Under the assumption that these processes are thermal, the absence of a strong e--e+ annihilation feature places constraints on the compactness (L/R ratio) of these sources. Observations favor sources of small compactness ratio. 13 references, 3 figures
Additional details
Publishing Information
- Journal Title
- AIP Conf. Proc.
- Journal Issue
- no.101
- Series
- AIP Conf. Proc.
- ISSN
- 0094-243X
Conference
- Title
- Workshop on positron-electron pairs in astrophysics.
- Dates
- 6-8 Jan 1983.
- Place
- Greenbelt, MD (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 16062610
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANNIHILATION; BACKGROUND RADIATION; BREMSSTRAHLUNG; COSMIC PHOTONS; COSMIC X-RAY SOURCES; ELECTRONS; ENERGY SPECTRA; PAIR PRODUCTION; POSITRONS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; COSMIC RADIATION; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; PHOTONS; RADIATIONS; SPECTRA
Optional Information
- Secondary number(s)
- CONF-830136--.