High-energy phase diagrams with charge and isospin axes under heavy-ion collision and stellar conditions

K. Aryal, C. Constantinou, R. L. S. Farias, and V. Dexheimer
Phys. Rev. D 102, 076016 – Published 27 October 2020

Abstract

We investigate the phase transition from hadron to quark matter in the general case without the assumption of chemical equilibrium. The effects of net strangeness on charge and isospin fractions, chemical potentials, and temperature are studied in the context of the Chiral Mean Field (CMF) model that incorporates chiral symmetry restoration and deconfinement. The extent to which these quantities are probed during deconfinement in conditions expected to exist in protoneutron stars, binary neutron-star mergers, and heavy-ion collisions is analyzed via the construction of 3-dimensional phase diagrams.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Received 11 April 2020
  • Revised 20 July 2020
  • Accepted 1 October 2020

DOI:https://doi.org/10.1103/PhysRevD.102.076016

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Nuclear PhysicsParticles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

K. Aryal1, C. Constantinou1, R. L. S. Farias2, and V. Dexheimer1

  • 1Department of Physics, Kent State University, Kent, Ohio 44243, USA
  • 2Departamento de Física, Universidade Federal de Santa Maria, 97105-900 Santa Maria, Rio Grande do Sul, Brazil

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 102, Iss. 7 — 1 October 2020

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×