Thomas–Fermi approximation in the phase transition of neutron star matter from β-stable nuclear matter to quark matter
Author:
Funder
University of Kashan, Iran
Publisher
Elsevier BV
Subject
General Physics and Astronomy
Reference58 articles.
1. Compact Stars, Nuclear Physics, Particle Physics, and General Relativity;Glendenning,2000
2. Black Holes, White Dwarfs and Neutron Stars;Shapiro,2008
3. First-order phase transitions with more than one conserved charge: Consequences for neutron stars
4. Hybrid stars with the color dielectric and the MIT bag models
5. Strange quark matter and compact stars
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