Excluded volume effects in the hybrid star EoS

15th International Conference on Strangeness in Quark Matter

Alvarez-Castillo, David E.^1,2 ; Kaltenborn, Mark A. R.^3 ; Blaschke, David^1,3,4

Bogoliubov Laboratory for Theoretical Physics, JINR Dubna, Dubna

141980, Russia^1

Universidad Autónoma de San Luis Potosí, S.L.P., México

78290, Mexico^2

Instytut Fizyki Teoretycznej, Uniwersytet Wroclawski, Wroclaw

50-204, Poland^3

National Research Nuclear University (MEPhI), Moscow

115409, Russia^4

关键词: Deconfinement;    Density functionals;    Electric neutrality;    Equation of state;    Excluded volume;    Excluded volume effects;    Nuclear matters;    String tension;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/668/1/012035/pdf
DOI  :  10.1088/1742-6596/668/1/012035

来源: IOP

【 摘 要 】

In this contribution, we outline a new 2-phase description of the quark-nuclear matter hybrid equation of state that takes into account effects of phase space occupation (excluded volume) in both, the hadronic and the quark matter phases. For the nuclear matter phase, the reduction of the available volume at increasing density leads to a stiffening, while for the quark matter phase a reduction of the effective string tension in the confining density functional is obtained. The deconfinement phase transition in the resulting hybrid equation of state is sensitive to both excluded volume effects. As an application, we consider matter under compact star constraints of electric neutrality and β-equilibrium. We obtain mass- radius relations for hybrid stars that fulfill the 2M constraint and exhibit the high-mass twin phenomenon. Both features depend sensitively on the excluded volume.