One possible mechanism for massive neutron star supported by soft EOS

Details One possible mechanism for massive neutron star supported by soft EOS One possible mechanism for massive neutron star supported by soft EOS

2012-04-13

arxiv.org/abs/1204.3030v1

IJMPD, Vol. 21, No. 4 (2012) 1250036

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

5 pages, 3 figures

Scientific paper

10.1142/S0218271812500368

The recently discovery of a massive neutron star (PSR J1614-2230 of $1.97\pm0.04M_{\odot}$) rules out the soft equation of states (EOSs) such as those included hyperons or kaon condensates at high densities, while the nuclear theory or the terrestrial laboratory data prefer a soft EOS. Here we propose one possible mechanism to allow that the observed massive neutron star can be supported by a soft EOS, that is, if the the gravitational constant $G$ varies at super strong field, a soft EOS can support the massive neutron stars.

Affiliated with

Also associated with

No associations

Rating

One possible mechanism for massive neutron star supported by soft EOS 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 One possible mechanism for massive neutron star supported by soft EOS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and One possible mechanism for massive neutron star supported by soft EOS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-144430