Published November 12, 2012
| Version v1
Journal article
Astrophysical and laboratory constraints for the dense matter equation of state
Creators
- 1. Dept. of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800 (United States)
Description
New measurements of neutron star masses and radii have lead to powerful constraints on the dense matter equation of state. In the vicinity of the nuclear saturation density, the symmetry energy is the least well understood aspect of the nuclear force. Independent constraints from a variety of nuclear experiments are now able to refine the parameters of the symmetry energy.
Additional details
Identifiers
- DOI
- 10.1063/1.4763414;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1484
- Journal Issue
- 1
- Journal Page Range
- p. 319-326
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Conference on origin of matter and evolution of galaxies 2011
- Dates
- 14-17 Nov 2011
- Place
- Wako (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44034848
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; EQUATIONS OF STATE; NEUTRON STARS; NUCLEAR FORCES; NUCLEAR MATTER; SYMMETRY
- Descriptors DEC
- EQUATIONS; MATTER; PHYSICS; STARS
Optional Information
- Notes
- (c) 2012 American Institute of Physics