Hybrid neutron stars in the mass‐radius diagram
- 29 June 2021
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 342 (5), 819-825
- https://doi.org/10.1002/asna.202114000
Abstract
No abstract availableKeywords
Funding Information
- Russian Foundation for Basic Research (18‐02‐40137)
This publication has 41 references indexed in Scilit:
- Hyperon-mixed neutron star with universal many-body repulsionThe European Physical Journal A, 2016
- Special point on the mass-radius diagram of hybrid starsAstronomy Letters, 2014
- Generic conditions for stable hybrid starsPhysical Review D, 2013
- Implications of the measurement of pulsars with two solar masses for quark matter in compact stars and heavy-ion collisions: A Nambu–Jona-Lasinio model case studyPhysical Review D, 2013
- Hadron–quark crossover and massive hybrid starsProgress of Theoretical and Experimental Physics, 2013
- Maximum mass of neutron stars and strange neutron-star coresAstronomy & Astrophysics, 2013
- Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiralPhysical Review D, 2010
- Phase diagram of three-flavor quark matter under compact star constraintsPhysical Review D, 2005
- Hybrid Stars that Masquerade as Neutron StarsThe Astrophysical Journal, 2005
- First-order phase transitions with more than one conserved charge: Consequences for neutron starsPhysical Review D, 1992