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Paper detail

Neutron Stars and the High Density Equation of State

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.

preprint2009arXivOpen access
T. KlahnC. D. RobertsD. B. BlaschkeF. Sandin
nucl-th
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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T. KlahnC. D. RobertsD. B. BlaschkeF. Sandin

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