3 citations · 3 across the 2 of their papers we have counts for
9 papers
Deconfinement Phase Transition under Chemical Equilibrium
Veronica Dexheimer, Krishna Aryal, Madison Wolf +2
In this work, we investigate how the assumption of chemical equilibrium with leptons affects the deconfinement phase transition to quark matter. This is done within the framework o…
3-Dimensional QCD Phase Diagrams for Strange Matter
V. Dexheimer, K. Aryal, C. Constantinou +1
In this work, we examine in detail the difference between constraining the electric charge fraction and isospin fraction when calculating the deconfinement phase transition in the…
High-Energy Phase Diagrams with Charge and Isospin Axes under Heavy-Ion Collision and Stellar Conditions
K. Aryal, C. Constantinou, R. L. S. Farias +1
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 iso…
Neutron-Star-Merger Equation of State
Veronica Dexheimer, Constantinos Constantinou, Elias R. Most +5
In this work, we discuss the dense matter equation of state (EOS) for the extreme range of conditions encountered in neutron stars and their mergers. The calculation of the propert…
Treating quarks within neutron stars
Sophia Han, M. A. A. Mamun, S. Lalit +2
Neutron star interiors provide the opportunity to probe properties of cold dense matter in the QCD phase diagram. Utilizing models of dense matter in accord with nuclear systematic…
The APR equation of state for simulations of supernovae, neutron stars and binary mergers
A. S. Schneider, C. Constantinou, B. Muccioli +1
Differences in the equation of state (EOS) of dense matter translate into differences in astrophysical simulations and their multi-messenger signatures. Thus, extending the number…