Probing the Equation of State of Dense Neutron-Rich Matter with High Energy Radioactive Beams

Details Probing the Equation of State of Dense Neutron-Rich Matter with High Energy Radioactive Beams Probing the Equation of State of Dense Neutron-Rich Matter with High Energy Radioactive Beams

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..dnp.be010l&link_type=abstract

American Physical Society, Division of Nuclear Physics Fall Meeting, October 30 - November 1, 2003, Tucson, Arizona, MEETING ID:

Physics

Nuclear Physics

Scientific paper

The equation of state (EOS) of dense neutron-rich matter has many important astrophysical implications on, such as, the nucleosynthesis in pre-supernova evolution of massive stars, mechanisms of supernova explosion, cooling mechanisms of protoneutron stars, kaon condensation and quark-hadron phae transition in neutron stars. However, our knowledge about the EOS of neutron-rich matter, especially at high densities, remains very poor. Nuclear reactions induced by high energy radioactive beams provide a unique opportunity to extract crucial information about the EOS of dense neutron-rich matter. In this talk, several promising probes of the EOS of dense neutron-rich matter based on isospin- and momentum-dependent transport theory, will be discussed.

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