The physics of dense nuclear matter from supernovae to quark gluon plasma

Details The physics of dense nuclear matter from supernovae to quark gluon plasma The physics of dense nuclear matter from supernovae to quark gluon plasma

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.337..319s&link_type=abstract

Nature (ISSN 0028-0836), vol. 337, Jan. 26, 1989, p. 319-324.

Astronomy and Astrophysics

Astrophysics

18

Dense Plasmas, Gluons, Neutron Stars, Nuclear Astrophysics, Quarks, Supernovae, Big Bang Cosmology, Coulomb Collisions, Electromagnetic Interactions, Equations Of State, Relativistic Theory

Scientific paper

Results of research on nuclear matter at high density created by heavy nuclear projectiles colliding head-on at relativistic energy are discussed. The nuclear equation of state is reviewed, and shock compression in relativistic collisions is examined. The results show that, at high density, nuclear matter is better regarded as a dense fluid rather than a collection of individual protons and neutrons. The significance of the findings for astrophysics and for quark matter is addressed.

Affiliated with

Also associated with

No associations

Rating

The physics of dense nuclear matter from supernovae to quark gluon plasma 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 physics of dense nuclear matter from supernovae to quark gluon plasma, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The physics of dense nuclear matter from supernovae to quark gluon plasma will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828131