[Submitted on 17 Nov 2018]
Sound velocity and tidal deformability in compact stars
Yong-Liang Ma🇨🇳 · Mannque Rho🇫🇷
The sound velocity and dimensionless tidal deformability are analyzed using the pseudo-conformal model we developed before. In contrast to the conclusion obtained in the previous works in the literature, our model with the upper bound of the sound velocity , the so-called conformal sound velocity, set in at a { density relevant to compact stars} where is the normal nuclear matter density, can accommodate {\it all} presently established nuclear matter and compact-star properties including the maximum star-mass constraint . This observation is associated with a possible emergence of pseudoconformal structure in compact star matter---in which the trace of energy-momentum tensor is a nearly density-independent nonzero constant---brought in by a topology change at commensurate with a possible change of degrees of freedom from hadrons.
- Comments:
- Version to appear in Phys. Rev. D
- Subjects:
- Nuclear Theory (nucl-th); High Energy Physics — Theory (hep-th)
- arXiv:
- 1811.07071 [pdf]