Friday, July 26, 2013

1307.6714 (Jochen Wambach)

Neutron Star Matter    [PDF]

Jochen Wambach
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.
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