Color superconductivity in compact stellar hybrid configurations

The discovery of pulsars PSR J1614-2230 and PSR J0348+0432 with masses of around 2M<sub>ʘ</sub> imposes strong constraints on the equations of state of cold, ultradense matter. If a phase transition from hadronic matter to quark matter were to occur in the inner cores of such massive neu...

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Detalles Bibliográficos
Autores principales:	Ranea Sandoval, Ignacio Francisco, Orsaria, Milva Gabriela, Han, Sophia, Weber, Fridolin, Spinella, William M.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2017
Materias:	Ciencias Astronómicas Nuclear matter in neutron stars Asymmetric nuclear matter Equations of state of nuclear matter Nuclear astrophysics Neutron stars
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/87239
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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