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Title: Rotating compact star with superconducting quark matter

Abstract

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.

Authors:
 [1];  [2];  [1]
  1. Indian Institute of Astrophysics, Koramangala, Bangalore-560034 (India)
  2. (India)
Publication Date:
OSTI Identifier:
20771305
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review. C, Nuclear Physics; Journal Volume: 73; Journal Issue: 2; Other Information: DOI: 10.1103/PhysRevC.73.025807; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; COLOR MODEL; COUPLING; EQUATIONS OF STATE; FLAVOR MODEL; MASS; MESONS; QUARK MATTER; QUARKS; STARS; SUPERCONDUCTIVITY

Citation Formats

Panda, P.K., Institute of Physics, Bhubaneswar-751005, and Nataraj, H.S. Rotating compact star with superconducting quark matter. United States: N. p., 2006. Web. doi:10.1103/PhysRevC.73.025807.
Panda, P.K., Institute of Physics, Bhubaneswar-751005, & Nataraj, H.S. Rotating compact star with superconducting quark matter. United States. doi:10.1103/PhysRevC.73.025807.
Panda, P.K., Institute of Physics, Bhubaneswar-751005, and Nataraj, H.S. Wed . "Rotating compact star with superconducting quark matter". United States. doi:10.1103/PhysRevC.73.025807.
@article{osti_20771305,
title = {Rotating compact star with superconducting quark matter},
author = {Panda, P.K. and Institute of Physics, Bhubaneswar-751005 and Nataraj, H.S.},
abstractNote = {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.},
doi = {10.1103/PhysRevC.73.025807},
journal = {Physical Review. C, Nuclear Physics},
number = 2,
volume = 73,
place = {United States},
year = {Wed Feb 15 00:00:00 EST 2006},
month = {Wed Feb 15 00:00:00 EST 2006}
}
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