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Neutron star structure from QCD

In this review article, we argue that our current understanding of the thermodynamic properties of cold QCD matter, originating from first principles calculations at high and low densities, can be used to efficiently constrain the macroscopic properties of neutron stars. In particular, we demonstrat...

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Detalles Bibliográficos
Autores principales: Fraga, Eduardo S, Kurkela, Aleksi, Vuorinen, Aleksi
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epja/i2016-16049-6
http://cds.cern.ch/record/2045940