Quark Deconfinement in Rotating Neutron Stars
In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective model of Quantum Chromodynamics (QCD) at low energies, to investigate the existence of deconfined quarks in the cores of neutron stars. Particular emphasis is put on the possible existence of quark m...
Guardado en:
| Autores principales: | Mellinger, Richard D., Weber, Fridolin, Spinella, William, Contrera, Gustavo Aníbal, Orsaria, Milva Gabriela |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82203 |
| Aporte de: |
Ejemplares similares
-
Phases of Hadron-Quark Matter in (Proto) Neutron Stars
por: Weber, Fridolin, et al.
Publicado: (2019) -
Structure of quark stars
por: Weber, Fridolin, et al.
Publicado: (2012) -
Neutrino Emissivity in the Quark-Hadron Mixed Phase
por: Spinella, William, et al.
Publicado: (2018) -
Rotation-driven phase transitions in the cores of pulsars
por: Mellinger, Richard D., et al.
Publicado: (2017) -
Quark-hadron Phase Transition in Proto-Neutron Stars Cores based on a Non-local NJL Model
por: Malfatti, Germán, et al.
Publicado: (2017)