Advances in High Energy Physics / 2009 / Article / Tab 1

Research Article

The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars

Table 1

Properties of nuclear matter and ( ), ( ) neutron stars. The properties of symmetric nuclear matter connected with isospin-asymmetric, beta-equilibrium matter ( ) whose EOS produces are listed. The coupling constants are chosen from the data in the paper [20, 21].

(MeV)
9.32610.4214.76510.020.020.04.0018.0

0.0130.0489.06310.8007.567

(MeV) (MeV)
0.701.021.0132930.0

We are committed to sharing findings related to COVID-19 as quickly and safely as possible. Any author submitting a COVID-19 paper should notify us at help@hindawi.com to ensure their research is fast-tracked and made available on a preprint server as soon as possible. We will be providing unlimited waivers of publication charges for accepted articles related to COVID-19. Sign up here as a reviewer to help fast-track new submissions.