Published June 2011
| Version v1
Journal article
Region of a hadron-quark mixed phase in hybrid stars
Creators
- 1. Division of Physics, Department of General Education, Kagawa National College of Technology, 355 Chokushi-cho, Takamatsu, Kagawa 761-8058 (Japan)
Description
Hadron-quark mixed phase is expected in a wide region of the inner structure of hybrid stars. However, we show that the hadron-quark mixed phase should be restricted to a narrower region because of the charge screening effect. The narrow region of the mixed phase seems to explain physical phenomena of neutron stars such as the strong magnetic field and glitch phenomena, and it would give a new cooling curve for the neutron star.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.83.068801;
- arXiv
- arXiv:1105.2445v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 83
- Journal Issue
- 6
- Journal Page Range
- p. 068801-068801.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42094654
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COOLING; HADRONS; MAGNETIC FIELDS; NEUTRON STARS; QUARKS; SCREENING
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; STARS
Optional Information
- Notes
- (c) 2011 American Institute of Physics