The Many Faces-and Phases-of Neutron Stars

Details The Many Faces-and Phases-of Neutron Stars The Many Faces-and Phases-of Neutron Stars

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..947..356p&link_type=abstract

VII LATIN AMERICAN SYMPOSIUM ON NUCLEAR PHYSICS AND APPLICATIONS. AIP Conference Proceedings, Volume 947, pp. 356-363 (2007).

Physics

Nuclear Physics

Nuclear Matter Aspects Of Neutron Stars, Nuclear Matter, Neutron Stars, Relativistic Heavy-Ion Collisions

Scientific paper

Understanding the equation of state (EOS) of nuclear matter is a central goal of nuclear physics that cuts across a variety of disciplines. Indeed, the limits of nuclear existence, the collision of heavy ions, the structure of neutron stars, and the dynamics of core-collapse supernova, all depend critically on the equation of state of hadronic matter. In this contribution I will concentrate on the EOS of cold baryonic matter with special emphasis on its impact on the structure and dynamics of neutron stars. In particular, I will discuss the many fascinating phases that one encounters as one travels from the low-density crust to the high-density core.

Affiliated with

Also associated with

No associations

Rating

The Many Faces-and Phases-of Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Many Faces-and Phases-of Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Many Faces-and Phases-of Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-824730