1303.1956 (Taparati Gangopadhyay et al.)

Strange star equation of state fits the refined mass measurement of 12 pulsars and predicts their radii    [PDF]

Taparati Gangopadhyay, Subharthi Ray, Xiang-Dong Li, Jishnu Dey, Mira Dey

There are three categories of stars whose masses have been found accurately in recent times: (1) two for which Shapiro delay is used which is possible due to GR light bending as the partner is heavy : PSR J1614-2230 and PSR J1903+0327 (2) six eclipsing stars for which numerical Roche Lobe geometry is used and (3) 3 stars for which spectroscopic methods are used and in fact for these three the mass and radii both are estimated. Motivated by large color (N_c) expansion using a modified Richardson potential, along with density dependent quark masses thereby allowing chiral symmetry restoration, we get compact strange stars fitting all the observed masses.

View original: http://arxiv.org/abs/1303.1956