Published March 23, 2001
| Version v1
Journal article
Chirally protected pion mass
Creators
- 1. Department of Physics and Astronomy, University of South Carolina, Columbia South Carolina 29208 (United States)
- 2. Department of Physics, Sookmyung Women's University, Seoul 140-742 (Korea, Republic of)
- 3. Department of Physics, Seoul National University, Seoul 151-742 (Korea, Republic of)
Description
The pion mass in the nuclear matter is protected by the chiral symmetry, which makes the existence of the S-wave pion condensation in the neutron star most unlikely. Some subtleties related to the calculation by the heavy baryon chiral perturbation theory of the pion mass in the dense matter are discussed
Additional details
Identifiers
- DOI
- 10.1063/1.1368274;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 556
- Journal Issue
- 1
- Journal Page Range
- p. 172-177
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 1. KIAS astrophysics workshop on explosive phenomena in astrophysical compact objects
- Dates
- 24-27 May 2000
- Place
- Seoul (Korea, Republic of)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35060175
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BARYONS; CHIRAL SYMMETRY; MASS; NEUTRON STARS; NUCLEAR MATTER; PIONS; S WAVES
- Descriptors DEC
- BOSONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; MATTER; MESONS; PARTIAL WAVES; PSEUDOSCALAR MESONS; STARS; SYMMETRY
Optional Information
- Notes
- (c) 2001 American Institute of Physics.