Published April 2005
| Version v1
Journal article
Neutron star properties from an NJL model modified to simulate confinement
Creators
- 1. Special Research Centre for the Subatomic Structure of Matter, University of Adelaide, Adelaide SA 5005 (Australia)
- 2. Department of Physics, School of Science, Tokai University, 117 Kita-Kaname, Hiratsuka 259-1207 (Japan)
- 3. Jefferson Lab, 12000 Jefferson Avenue, Newport News, VA 23606 (United States)
Description
The NJL model has recently been extended with a method to simulate confinement. This leads in mean field approximation to a natural mechanism for the saturation of nuclear matter. We use the model to investigate the equation of state of asymmetric nuclear matter and then use it to compute the properties of neutron stars
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2004.12.005;
- arXiv
- arXiv:nucl-th/0409073v1;
- PII
- S0920-5632(04)01017-5;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 141
- Journal Page Range
- p. 29-33
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- QCD Down Under
- Acronym
- Workshop on quantum chromodynamics
- Dates
- 10-19 Mar 2004
- Place
- Adelaide (Australia)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37102732
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- APPROXIMATIONS; ASYMMETRY; EQUATIONS OF STATE; MEAN-FIELD THEORY; NEUTRON STARS; NUCLEAR MATTER
- Descriptors DEC
- CALCULATION METHODS; EQUATIONS; MATTER; STARS
Optional Information
- Copyright
- Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.