pith. sign in

arxiv: 0810.2368 · v1 · pith:WBEOS5P3new · submitted 2008-10-14 · 🌌 astro-ph · hep-ph· nucl-th

Structure of Neutron Star with a Quark Core

G.H. Bordbar , M. Bigdeli , T. Yazdizadeh This is my paper
classification 🌌 astro-ph hep-phnucl-th
keywords equationneutronquarkstarstatecorestructureaffected
0
0 comments X
read the original abstract

The equation of state of de-confined quark matter within the MIT bag model is calculated. This equation of state is used to compute the structure of a neutron star with quark core. It is found that the limiting mass of the neutron star is affected considerably by this modification of the equation of state. Calculations are carried out for different choices of the bag constant.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Neutrino diagnostics of hadron-quark phase transition in Neutron Stars

    astro-ph.HE 2025-10 unverdicted novelty 4.0

    Neutrino light curves from neutron stars may show an enhanced peak-to-plateau ratio, a density-tracing delay, and transient spectral hardening as diagnostics of hadron-quark phase transitions on 10-50 ms timescales.