Neutron Star Versus Heavy-Ion Data:. is the Nuclear Equation of State Hard or Soft?

Details Neutron Star Versus Heavy-Ion Data:. is the Nuclear Equation of State Hard or Soft? Neutron Star Versus Heavy-Ion Data:. is the Nuclear Equation of State Hard or Soft?

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008esnm.conf..207s&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

Nuclear Equation Of State, Neutron Stars, Pulsars, Kaon Production In Heavy-Ion Collisions

Scientific paper

Recent astrophysical observations of neutron stars and heavy-ion data are confronted with our present understanding of the equation of state of dense hadronic matter. Emphasis is put on the possible role of the presence of hyperons in the interior of compact stars. We argue that data from low-mass pulsars provide an important cross-check between high-density astrophysics and heavy-ion physics.

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