Nuclear constraints on properties of rotating neutron stars and gravitational waves

Details Nuclear constraints on properties of rotating neutron stars and gravitational waves Nuclear constraints on properties of rotating neutron stars and gravitational waves

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..cal.c3001k&link_type=abstract

American Physical Society, 2010 Annual Meeting of the California-Nevada Section of the APS, October 29-30, 2010, abstract #C3.00

Physics

Nuclear Physics

Scientific paper

Nuclear reactions with radioactive beams provide unique means to constrain the equation of state (EOS) of neutron-rich matter, in particular its density dependence through the nuclear symmetry energy. The EOS is important for our understanding of numerous phenomena in nuclear physics, astrophysics and cosmology. Applying an EOS with symmetry energy constrained by recent nuclear laboratory data, we set a limit on the properties of rotating neutron stars and the resultant gravitational waves.

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