Quark matter at the interior of neutron stars

Details Quark matter at the interior of neutron stars Quark matter at the interior of neutron stars

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf..251o&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

Scientific paper

The density at the center of a neutron star reaches several times nuclear matter saturation density. At this density, the properties of strongly interacting matter are not well known. Exotic phases, such as hyperon matter, can appear. It is even possible that there is a phase transition to deconfined quark matter. Recent studies suggest that the phase structure of QCD in this domain is very rich. I will present the main characteristics of quark matter at high density as well as some observable consequences.

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