Astrophysical Measurement of the Equation of State of Neutron Star Matter

Details Astrophysical Measurement of the Equation of State of Neutron Star Matter Astrophysical Measurement of the Equation of State of Neutron Star Matter

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21830201o&link_type=abstract

American Astronomical Society, AAS Meeting #218, #302.01; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astrophysics

Scientific paper

Neutron stars offer the unique possibility of probing the equation of state of cold, ultradense matter. Using the recent measurements of neutron star radii and masses, I will present the first astrophysical inference of the pressure of cold matter above nuclear saturation density. I will discuss the implications of this measurement for nuclear theory as well as its astrophysical implications for supernovae and gravitational waves.

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