activity
20062026
most citedElectrically Charged Strange Quark Stars

169 citations · 1.2k across the 52 of their papers we have counts for

collaborators

54 papers

nucl-th2026

S-wave kaon condensation in neutron-star matter within a chiral model framework with dynamical meson masses

Yuhan Wang, Rajesh Kumar, Joaquin Grefa +4

We investigate s-wave kaon condensation in dense matter and neutron stars within the updated Chiral Mean Field model with an improved meson description (mCMF), which incorporates d…

astro-ph.HE2026

Enhanced Neutrino Cooling from Parity-Doubled Nucleons in Neutron Star Cooling Simulations

Rodrigo Negreiros, Liam Brodie, Jan Steinheimer +2

Although restoration of chiral symmetry is predicted by quantum chromodynamics to take place at high baryon density, most modeling of neutron star interiors disregards a chiral pha…

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.HE2024★ 4 cited

Rotational Properties of Inverted Hybrid Stars

Rodrigo Negreiros, Chen Zhang, Renxin Xu

We study the rotational properties of inverted hybrid stars (also termed cross stars), which have been recently proposed as a possible new class of compact stars characterized by a…

astro-ph.HE2024

Fast Pulsars, Neutron Stars, and Astrophysical Strange Quark Matter Objects

Delaney Farrell, Fridolin Weber, Milva G. Orsaria +5

This book chapter explores key aspects of neutron stars, pulsar glitches, tidal deformability, fast pulsars, the equation of state, and strange quark matter stars. Challenges in di…

astro-ph.HE2023★ 83 cited

What is the nature of the HESS J1731-347 compact object?

Violetta Sagun, Edoardo Giangrandi, Tim Dietrich +3

Once further confirmed in future analyses, the radius and mass measurement of HESS J1731-347 with and will be amo…