Proton fraction in neutron stars

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 Pgaes in REVTex, 2 Figures, 1 Table

Scientific paper

10.1088/0256-307X/18/1/350

The proton fraction in ${\sl \beta}$-stable neutron stars is investigated within the framework of the Skyrme-Hartree-Fock theory using the extended Skyrme effective interaction for the first time. The calculated results show that the proton fraction disappears at high density, which implies that the pure neutron matter may exist in the interior of neutron stars. The incompressibility of the nuclear equation of state is shown to be more important to determine the proton fraction. Meanwhile, it is indicated that the addition of muons in neutron stars will change the proton fraction. It is also found that the higher-order terms of the nuclear symmetry energy have obvious effects on the proton fraction and the parabolic law of the nuclear symmetry energy is not enough to determine the proton fraction.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Proton fraction in 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 Proton fraction in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Proton fraction in neutron stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-708086

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.