Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections

T Dietrich, T Hinderer, A Samajdar - General Relativity and Gravitation, 2021 - Springer
Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …

Electromagnetic probes: Theory and experiment

F Geurts, RA Tripolt - Progress in Particle and Nuclear Physics, 2023 - Elsevier
We review the current state of research on electromagnetic probes in the context of heavy-
ion collisions. The focus is on thermal photons and dileptons which provide unique insights …

Was GW170817 a canonical neutron star merger? Bayesian analysis with a third family of compact stars

D Blaschke, A Ayriyan, DE Alvarez-Castillo… - Universe, 2020 - mdpi.com
We investigate the possibility that GW170817 was not the merger of two conventional
neutron stars (NS), but involved at least one if not two hybrid stars with a quark matter core …

Equation of state for hot QCD and compact stars from a mean-field approach

A Motornenko, J Steinheimer, V Vovchenko… - Physical Review C, 2020 - APS
The thermodynamic properties of high temperature and high density QCD matter are
explored within the chiral SU (3)-flavor parity-doublet Polyakov-loop quark-hadron mean …

Neutron star matter based on a parity doublet model including the meson

YK Kong, T Minamikawa, M Harada - Physical Review C, 2023 - APS
We study the effect of the isovector-scalar meson a 0 (980) on the properties of nuclear
matter and the neutron star (NS) matter by constructing a parity doublet model with including …

Remarks on nuclear matter: How an condensate can spike the speed of sound, and a model of baryons

RD Pisarski - Physical Review D, 2021 - APS
I make two comments about nuclear matter. First, I consider the effects of a coupling
between the O (4) chiral field, ϕ→, and the ω μ meson,∼+ ϕ→ 2 ω μ 2; for any net baryon …

SU (3) parity doubling in cold neutron star matter

ES Fraga, R da Mata, J Schaffner-Bielich - Physical Review D, 2023 - APS
We present a phenomenological model to investigate the chiral phase transition
characterized by parity doubling in dense, beta equilibrated, cold matter. Our model …

Chiral symmetry restoration and matter formation in neutron stars

M Marczenko, K Redlich, C Sasaki - Physical Review D, 2022 - APS
We analyze the effects of chiral symmetry restoration in hadronic matter, including the lowest-
lying baryonic resonance Δ based on the parity doublet model. We study the role of Δ and its …

Hot quark matter and (proto-) neutron stars

G Malfatti, MG Orsaria, GA Contrera, F Weber… - Physical Review C, 2019 - APS
In the first part of this paper, we use a nonlocal extension of the three-flavor Polyakov-
Nambu-Jona-Lasinio model, which takes into account flavor-mixing, momentum dependent …

Nonperturbative quark matter equations of state with vector interactions

K Otto, M Oertel, BJ Schaefer - The European Physical Journal Special …, 2020 - Springer
Nonperturbative equations of state (EoSs) for two and three quark flavors are constructed
with the functional renormalization group (FRG) within a quark-meson model truncation …