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Neutron Star Matter

In this presentation I discuss two aspects of the neutron-matter equation of state. One relates to the symmetry energy of nuclear matter and empirical constraints on its slope parameter at saturation density. The second deals with spatially inhomogeneous chiral phases of deconfined quark matter in the inner core of a neutron star.

4 nodes3 linksoverview mapNeutron Star Matter
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Neutron Star Matter4 visible / 4 total nodes / 3 links
AuthorshipTopic signalTopic signalWNeutron Star Matterpreprint / 2013AJochen WambachResearcherThep-ph13193 worksTnucl-th4595 works
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Neutron Star Matter

preprint / 2013

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