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arxiv: nucl-th/0612021 · v1 · submitted 2006-12-05 · ⚛️ nucl-th · astro-ph· hep-ph

Neutron stars and quark matter

classification ⚛️ nucl-th astro-phhep-ph
keywords matterneutronquarkstarsbeginchallengecloseconstrain
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Recent observations of neutron star masses close to the maximum predicted by nucleonic equations of state begin to challenge our understanding of dense matter in neutron stars, and constrain the possible presence of quark matter in their deep interiors.

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