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20072026
most citedTransport Coefficients of Hadronic Matter near

239 citations · 3.9k across the 138 of their papers we have counts for

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nucl-th2026

A 4D -expanded lattice QCD equation of state with a multi-dimensional 3D-Ising-type critical contribution

Francesco Di Clemente, Prachi Garella, Johannes Jahan +5

Inferring the possible existence and location of a critical point on the QCD phase diagram through experimental observations requires equations of state that include both lattice Q…

nucl-th2026

Searching for the QCD critical point with relativistic viscous hydrodynamics

Kevin P. Pala, Surkhab K. Virk, Isabella Danhoni +3

With the STAR's Beam Energy Scan II, a rich amount of data exists to search for the QCD critical point. However, a central challenge is that the critical point cannot be directly e…

nucl-th2026

MUSES workflows for pQCD constraints on dense matter with finite quark masses

Isabella Danhoni, Mateus Reinke Pelicer, Débora Mroczek +3

We present a modular implementation of next-to-leading order (NLO) perturbative QCD (pQCD) thermodynamics with finite strange quark mass in the MUSES Calculation Engine, enabling r…

nucl-th2026

How strange: Phase diagrams with 3 critical points

Mateus Reinke Pelicer, Nikolas Cruz Camacho, Rajesh Kumar +2

We show that the Chiral Mean-Field model (CMF) can produce a phase diagram with three critical points: the nuclear liquid-gas transition, quark deconfinement, and a strangeness dri…

astro-ph.HE2026

Strangeness Transport in Binary Neutron Star Mergers

Melvin Storbacka, Jiaxi Wu, Alexander Haber +5

The presence of hyperons in the cores of neutron stars opens fast strangeness equilibration channels that can produce bulk-viscous dissipation during binary inspiral. Because these…

nucl-th2026

Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties

Isaac Legred, Mateus Reinke Pelicer, Veronica Dexheimer +2

Chiral models of nuclear interactions provide approximate, phenomenological descriptions of dense matter that respect the symmetries of quantum chromodynamics. Their Lagrangian par…

nucl-th2026

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine

Johannes Jahan, Kevin P. Pala, Yumu Yang +42

The equation of state of hot and dense matter is essential for describing heavy-ion collisions at all collision energies. Here, we explore the capabilities of the latest version of…

gr-qc2026

Donutization Inside Neutron Stars: Shell-Localized Scalar Fields

Hao-Jui Kuan, Alan Tsz-Lok Lam, Jacquelyn Noronha-Hostler +1

Heavy scalar fields ( eV) in scalar-tensor gravity are expected to be hidden from neutron-star observations because their Compton wavelength is sub-stellar. We s…

nucl-th2026

Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state

Nikolas Cruz-Camacho, Carlos Conde-Ocazionez, Veronica Dexheimer +2

The equation of state of matter at supranuclear densities governs the astrophysical observables of neutron stars. A realistic, though complex, description is provided by the Chiral…

gr-qc2026

Dynamical tidal response of neutron stars as a probe of dense-matter properties

Abhishek Hegade K. R., Yumu Yang, Mauricio Hippert +3

Dynamical tidal deformations play a crucial role in the gravitational waves emitted by binary neutron star systems during their late inspiral. In this work, we systematically explo…

nucl-th2026

Mesoscopic chemical potentials across the (hyper)nuclear landscape

Jacquelyn Noronha-Hostler

Finite nuclei constrain the dense-matter equation of state (EOS), yet they are self-bound quantum droplets far from the thermodynamic limit. Motivated by an analogy to quantum dots…