Rotating compact star with superconducting quark matter
Journal Article
·
· Physical Review. C, Nuclear Physics
- Indian Institute of Astrophysics, Koramangala, Bangalore-560034 (India)
A compact star with a superconducting quark core, a hadron crust, and a mixed phase between the two is considered. The quark-meson coupling model for hadron matter and the color-flavor-locked quark model for quark matter is used to construct the equation of state for the compact star. The effect of pairing of quarks in the color-flavor-locked phase and the mixed phase on the mass, radius, and period of the rotating star is studied.
- OSTI ID:
- 20771305
- Journal Information:
- Physical Review. C, Nuclear Physics, Vol. 73, Issue 2; Other Information: DOI: 10.1103/PhysRevC.73.025807; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2813
- Country of Publication:
- United States
- Language:
- English
Similar Records
Massive neutron stars with a color superconducting quark matter core
Phase diagram of three-flavor quark matter under compact star constraints
Constraining phases of quark matter with studies of r-mode damping in compact stars
Journal Article
·
Tue May 19 00:00:00 EDT 2020
· Physical Review C
·
OSTI ID:20771305
Phase diagram of three-flavor quark matter under compact star constraints
Journal Article
·
Thu Sep 15 00:00:00 EDT 2005
· Physical Review. D, Particles Fields
·
OSTI ID:20771305
+2 more
Constraining phases of quark matter with studies of r-mode damping in compact stars
Journal Article
·
Mon Nov 15 00:00:00 EST 2010
· Physical Review. C, Nuclear Physics
·
OSTI ID:20771305