[Submitted on 2 Feb 2017] (cross-list from astro-ph.HE)
Bayesian analysis for a new class of hybrid EoS models using mass and radius data of compact stars
A. Ayriyan🇷🇺 · D. E. Alvarez-Castillo🇷🇺 · S. Benic🇯🇵 · D. Blaschke🇷🇺 · H. Grigorian🇦🇲 · S. Typel🇩🇪
We present a Bayesian analysis for a new class of realistic models of two-phase equations of state (EoS) for hybrid stars and demonstrate that the observation of a pair of high-mass twin stars would have a sufficient discriminating power to favor hybrid EoS with a strong first order phase transition over alternative EoS. Such a measurement would provide evidence for the existence of a critical endpoint in the QCD phase diagram.
- Comments:
- 6 pages, 2 figures, 1 scheme, contribution to the Proceedings of the International Conference on Critical Point and Onset of Deconfinement (CPOD'2016), Wroclaw, Poland, May 29 - June 5, 2016
- Subjects:
- High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
- arXiv:
- 1702.00801 [pdf]