On the possibility of stable quark and pion-condensed stars
- 1 November 1981
- journal article
- Published by IOP Publishing in Journal of Physics A: General Physics
- Vol. 14 (11) , L471-L475
- https://doi.org/10.1088/0305-4470/14/11/009
Abstract
The conditions for the appearance of stable quark stars and pion-condensed stars are analysed. On the basis of recently suggested equations of state such configurations can exist either as a third stable family or as a separated part of the stable neutron star branch.Keywords
This publication has 21 references indexed in Scilit:
- On the neutron star transition to a pion-condensed configurationPhysics Letters B, 1980
- Note on the neutron matter-quark matter transitionPhysics Letters B, 1980
- Possible existence of quark starsJournal of Physics A: General Physics, 1979
- (Non)-Abelian gauge field theories of the Fermi gas. Neutron-quark starsPhysics Letters B, 1978
- Asymptotic freedom and the baryon-quark phase transitionPhysical Review D, 1977
- On the possibility of stable quark starsThe Astrophysical Journal, 1977
- Can a neutron star be a giant MIT bag?Physics Letters B, 1976
- Pion condensed matter at high densities - Equation of state and stellar modelsThe Astrophysical Journal, 1975
- Equation of State at Supranuclear Densities and the Existence of a Third Family of Superdense StarsPhysical Review B, 1968
- A Catalogue of Methods for Studying the Normal Modes of Radial Pulsation of General-Relativistic Stellar ModelsThe Astrophysical Journal, 1966