Published November 2006
| Version v1
Journal article
Quark deconfinement in neutron stars and gamma-ray bursts
Creators
- 1. Dipartimento di Fisica 'E. Fermi', Universita di Pisa and INFN sezione di Pisa. Largo Bruno Pontecorvo 3, I-56127 Pisa (Italy)
Description
We discuss a model for the energy source of gamma-ray burst which is based on the 'delayed conversion' of a metastable pure hadronic compact star ('neutron star') to a quark star (hybrid star or strange star)
Availability note (English)
Available online at http://stacks.iop.org/1742-6596/50/208/jpconf6_50_024.pdf or at the Web site for the Journal of Physics. Conference Series (Online) (ISSN 1742-6596) http://www.iop.org/Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 50
- Journal Issue
- 1
- Journal Page Range
- p. 208-215
- ISSN
- 1742-6596
Conference
- Title
- 5. international conference on physics and astrophysics of quark gluons
- Dates
- 8-12 Feb 2005
- Place
- Salt Lake City, Kolkata (India)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38033474
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BAG MODEL; COSMIC GAMMA BURSTS; HADRONS; NEUTRON STARS; QUARKS; STRANGENESS
- Descriptors DEC
- COMPOSITE MODELS; COSMIC RADIATION; ELEMENTARY PARTICLES; EXTENDED PARTICLE MODEL; FERMIONS; IONIZING RADIATIONS; MATHEMATICAL MODELS; PARTICLE MODELS; PARTICLE PROPERTIES; PRIMARY COSMIC RADIATION; QUARK MODEL; RADIATIONS; STARS