Three-body forces and neutron star structure

Details Three-body forces and neutron star structure Three-body forces and neutron star structure

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004phrvc..69a8801z&link_type=abstract

Physical Review C, vol. 69, Issue 1, id. 018801

Mathematics

Logic

66

Nuclear Matter, Nuclear Matter Aspects Of Neutron Stars, Many-Body Theory, Neutron Stars

Scientific paper

We calculate the nucleonic equation of state within the Brueckner-Bethe-Goldstone formalism using the Argonne υ18 two-body interaction and a three-body interaction. We adopt two different three-body forces: the phenomenological Urbana IX model and a microscopic meson-exchange force including nucleon virtual excitations and nucleon-antinucleon excitations. We compare their respective predictions regarding the structure of neutron stars, in particular the mass-radius relation.

Affiliated with

Also associated with

No associations

Rating

Three-body forces and neutron star structure 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 Three-body forces and neutron star structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-body forces and neutron star structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1553269