Dense Nuclear Matter:. Constraints from Neutron Stars

Details Dense Nuclear Matter:. Constraints from Neutron Stars Dense Nuclear Matter:. Constraints from Neutron Stars

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008esnm.conf..199l&link_type=abstract

EXOTIC STATES OF NUCLEAR MATTER. Proceedings of the International Symposium EXOCT07. Held 11-15 June 2007 in Catania University,

Physics

Neutron Stars, Equation Of State

Scientific paper

Neutron stars are a natural laboratory for the exploration of dense nuclear matter. Analytic constraints from general relativity, causality and stability provide a general framework into which specific constraints concerning dense matter properties can be made from measurements of masses, spin rates, thermal emissions, and quasi-periodic oscillations observed in accreting and bursting sources. Focus is placed upon recent mass and spin rate measurements and their implications for theory.

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