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nucl-th2024
BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics
Christopher Plumberg, Dekrayat Almaalol, Travis Dore +8
Conservation laws play a crucial role in the modeling of heavy-ion collisions, including the those for charges such as baryon number (B), strangeness (S), and electric charge (Q).…
astro-ph.HE2024
Validity of a finite temperature expansion for dense nuclear matter
Debora Mroczek, Nanxi Yao, Katherine Zine +5
In this work we provide a new, well-controlled expansion of the equation of state of dense matter from zero to finite temperatures () while covering a wide range of charge fract…
nucl-th2024
Bayesian analysis of nontrivial features in the speed of sound inside neutron stars in light of astrophysical and pQCD constraints
Debora Mroczek
Functional forms of the neutron star Equation of State (EoS) are required to extract the viable EoS band from neutron star observations. Realistic nuclear EoS, containing deconfine…