Neutron Stars and the High Density Equation of State

Details Neutron Stars and the High Density Equation of State Neutron Stars and the High Density Equation of State

2009-04-30

arxiv.org/abs/0904.4729v1

AIP Conf.Proc.1128:175-185,2009

Physics

Nuclear Physics

Nuclear Theory

10 pages, 6 figures, Proc. 5th ANL/MSU/JINA/INT FRIB Workshop on Bulk Nuclear Properties, E. Lansing, Nov. 19-22, 2008

Scientific paper

10.1063/1.3146212

One of the key ingredients to understand the properties of neutrons stars is the equation of state at finite densities far beyond nuclear saturation. Investigating the phase structure of quark matter that might be realized in the core of NS inspires theory and observation. We discuss recent results of our work to point out our view on challenges and possibilities in this evolving field by means of a few examples.

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