Some limits on excitation energies of nuclei in hot matter

Details Some limits on excitation energies of nuclei in hot matter Some limits on excitation energies of nuclei in hot matter

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..382m&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. 382-386.

Physics

Nuclear Physics

2

Atomic Excitations, Dense Plasmas, Gravitational Collapse, Nucleons, Stellar Structure, Matter (Physics), Nuclear Physics, Stellar Models

Scientific paper

The occupation probability of energetically separable states within a nucleus has been computed. This probability is used to estimate the overlap between nuclear partition functions and the external phase space of free nucleons. The results indicate that appreciable overlap is possible only at nuclear excitation energies that are at least an order of magnitude greater than the single particle's separation energy. These results confirm the existence of nuclei to nuclear densities during stellar collapse.

Affiliated with

Also associated with

No associations

Rating

Some limits on excitation energies of nuclei in hot matter 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 Some limits on excitation energies of nuclei in hot matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some limits on excitation energies of nuclei in hot matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-880231