Cargando…
Interacting quark matter equation of state for compact stars
Lattice QCD studies of the thermodynamics of the hot quark-gluon plasma (QGP) demonstrate the importance of accounting for the interactions of quarks and gluons, if one wants to investigate the phase structure of strongly interacting matter. Motivated by this observation and using state-of-the-art r...
Autores principales: | Fraga, Eduardo S., Kurkela, Aleksi, Vuorinen, Aleksi |
---|---|
Lenguaje: | eng |
Publicado: |
2013
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/2041-8205/781/2/L25 http://cds.cern.ch/record/1630331 |
Ejemplares similares
-
Neutron star structure from QCD
por: Fraga, Eduardo S, et al.
Publicado: (2015) -
Gravitational-wave constraints on the neutron-star-matter Equation of State
por: Annala, Eemeli, et al.
Publicado: (2017) -
QCD constraints on the equation of state for compact stars
por: Fraga, E S, et al.
Publicado: (2016) -
Evidence for quark-matter cores in massive neutron stars
por: Annala, Eemeli, et al.
Publicado: (2019) -
Cool quark matter
por: Kurkela, Aleksi, et al.
Publicado: (2016)