activity
20072026
most citedSignatures of quark-hadron phase transitions in general-relativistic neutron-star mergers

389 citations · 3.8k across the 122 of their papers we have counts for

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10 papers · 1 filter

nucl-th2025

Relativistic mean-field model with density- and isospin-density-dependent couplings

Gabriel Frohaug, Konstantin Maslov, Veronica Dexheimer +4

We present a new hadronic EoS with hyperons built within the relativistic mean-field (RMF) formalism with baryon-density- and isospin-density-dependent couplings. Motivated by micr…

astro-ph.HE2025★ 5 cited

Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers

P. Hammond, A. Clevinger, M. Albino +10

In this paper we investigate quark deconfinement in neutrons stars and their mergers, focusing on the effects of higher orders for the phase transition between hadronic and quark m…

astro-ph.HE2025★ 4 cited

Impact of magnetic field-driven anisotropies on the equation of state probed in neutron star mergers

Elias R. Most, Jeffrey Peterson, Luigi Scurto +2

Binary neutron star mergers can produce extreme magnetic fields, some of which can lead to strong magnetar-like remnants. While strong magnetic fields have been shown to affect the…

astro-ph.HE2025

Axisymmetric Cooling of Neutron Stars with Strong Magnetic Fields

Rodrigo Negreiros, Jeffrey Peterson, Veronica Dexheimer

We study the cooling evolution of neutron stars with strong poloidal magnetic fields (with strength not far from observed values) using the full general relativity 2-dimensional \t…

astro-ph.HE2025

Recurring region for neutron-star observables

Alexander Clevinger, Zidu Lin, Milena Albino +3

In this letter, we report a novel, somewhat analytical way to produce equations of state (EOSs) that generate particular values of neutron star mass, radius, and tidal deformabilit…

nucl-th2025

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars

Mateus Pelicer, Veronica Dexheimer, Joaquin Grefa

For densities beyond nuclear saturation, there is still a large uncertainty in the equations of state (EoS) of dense matter that translate into uncertainties in the internal struct…