Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine
Johannes Jahan🇺🇸 · Kevin P. Pala🇧🇷 · Yumu Yang🇺🇸 · Isabella Danhoni🇺🇸 · Prachi Garella🇺🇸 · Jonathan Gonzales🇺🇸 · Joaquin Grefa🇺🇸 · Mauricio Hippert🇧🇷 · Surkhab Kaur Virk · Micheal Kahangirwe🇺🇸 · Musa R. Khan🇺🇸 · Feyisola Nana and 33 other authors
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 the MUSES Calculation Engine, , focusing on software modules and workflows that compute the equation of state and observable properties of the matter produced in heavy-ion collisions. These include several equations of state, ranging from first-principles lattice QCD to phenomenological approaches, with or without a critical point, and with phase-space dimensionality ranging from two dimensions defined by temperature and baryon chemical potential , to four dimensions after the addition of strangeness and electric-charge chemical potentials and . We also discuss modules that provide additional thermodynamic quantities and observables relevant for heavy-ion modeling, including elements of the pressure Hessian matrix and transport coefficients. Workflow examples are constructed that merge two equations of state thermodynamically consistently to extend phase-diagram coverage, and feed the results into an equation of state inverter to produce inputs suitable for hydrodynamic simulations. Finally, we apply this framework to perform a relativistic viscous hydrodynamic simulation with equations of state with an extended and coverage and a movable critical point, including effects from transport coefficients that phenomenologically encode critical scaling, at collision energies , and GeV.