PaperPanorama

Nuclear Theory·nucl-th

Monday·December 16, 2024

10 papers5 primary·5 cross-listed

  1. 01

    Effective temperatures of the QGP from thermal photon and dilepton production

    Olaf Massen🇳🇱 · Govert Nijs🇨🇭 · Mike Sas🇳🇱 · Wilke van der Schee🇳🇱 · Raimond Snellings🇳🇱

    Thermal electromagnetic radiation is emitted by the quark-gluon plasma (QGP) throughout its space-time evolution, with production rates that depend characteristically on the temperature. We study this temperature using thermal photons and dileptons using the Trajectum heavy ion code, which is constrained by Bayesian analysis. In addition we present the elliptic flow of both the thermal photons and thermal dileptons including systematic uncertainties corresponding to the model parameter uncertainty. We give a comprehensive overview of the resulting effective temperatures , obtained from thermal photon transverse momentum and thermal dilepton invariant mass distributions, as well as the dependence of on various selection criteria of these probes. We conclude that the obtained from thermal photons is mostly insensitive to the temperature of the QGP with a value of 250-300 MeV depending on their transverse momentum, almost independent of collision centrality. Thermal dileptons are much better probes of the QGP temperature as they do not suffer from a blue shift as their invariant mass is used, allowing for a more precise constraint of the QGP temperature during different stages of the evolution of the system. By applying selection criteria on the dilepton transverse momentum and the invariant mass we are able to extract fluid temperatures on average times ranging from late emission (fm) to very early emissions (fm). Furthermore, we show how these selection criteria can be used to map the elliptic flow of the system all throughout its evolution.

    nucl-thhep-phnucl-exEPJC(2025)·17 citations
  2. 02

    Deuteron- scattering using nucleon- optical potentials fitted to four-body amplitudes

    A. Deltuva · D. Jurčiukonis

    Deuteron- reactions in the 15 to 40 MeV range are studied using a three-body model where the constructed nonlocal optical potentials rely on rigorous nucleon- scattering calculations. The differential cross section for the elastic scattering and neutron transfer reaction is predicted quite well up to 90 deg scattering angles. The importance of the Pauli term in complex potentials is demonstrated.

    nucl-thnucl-exPLB(2025)·0 citations
  3. 03

    Improving the predictive power of empirical shell-model Hamiltonians

    J. A. Purcell · B. A. Brown · B. C. He · S. R. Stroberg · W. B. Walters

    We present two developments which enhance the predictive power of empirical shell-model Hamiltonians for cases in which calibration data are sparse. A recent improvement in the ab initio derivation of effective Hamiltonians leads to a much better starting point for the optimization procedure. In addition, we introduce a protocol to avoid overfitting, enabling a more reliable extrapolation beyond available data. These developments will enable more robust predictions for exotic isotopes produced at rare isotope beam facilities and in astrophysical environments.

    nucl-thPRC(2025)·5 citations
  4. 04

    Relativistic Viscous Hydrodynamics in the Density Frame: Numerical Tests and Comparisons

    Jay Bhambure🇺🇸 · Aleksas Mazeliauskas🇩🇪 · Jean-Francois Paquet🇺🇸 · Rajeev Singh🇷🇴 · Mayank Singh🇺🇸 · Derek Teaney🇺🇸 · Fabian Zhou🇩🇪

    We conduct a numerical study of relativistic viscous fluid dynamics in the Density Frame for one-dimensional fluid flows. The Density Frame is a formulation of relativistic viscous hydrodynamics that is first-order in time, requires no auxiliary fields, and has no non-hydrodynamic modes. We compare our results to QCD kinetic theory simulations and find excellent agreement within the regime of applicability of hydrodynamics. Additionally, the Density Frame results remain well-behaved and robust near the boundary of applicability. We also compare our findings to the second-order-in-time hydrodynamic theory developed by Bemfica, Disconzi, Noronha, and Kovtun (BDNK) and a well-known Müller-Israel-Stewart-type hydrodynamics code, MUSIC, which is commonly used to simulate heavy-ion collisions.

    nucl-thgr-qcPRC(2025)·24 citations
  5. 05

    Stochastic relativistic viscous hydrodynamics from the Metropolis algorithm

    Jay Bhambure🇺🇸 · Rajeev Singh🇷🇴 · Derek Teaney🇺🇸

    We propose an algorithm for simulating stochastic relativistic fluid dynamics based on Metropolis updates. Each step of the algorithm begins with an update based on ideal hydrodynamics. This is followed by proposing random (spatial) momentum transfers between fluid cells, keeping the total energy fixed. These proposals are then accepted or rejected using the change in entropy as a statistical weight. The algorithm reproduces relativistic viscous hydrodynamics in the ``Density Frame", which is a formulation of viscous hydrodynamics we review and clarify here. This formulation is first order in time and requires no auxiliary dynamical fields such as . The only parameters are the shear and bulk viscosities and the equation of state. By adopting the 3+1 split of general relativity, we extend the Metropolis algorithm to general space-time coordinates, such as Bjorken coordinates, which are commonly used to simulate heavy-ion collisions.

    nucl-thgr-qchep-thPRC(2025)·21 citations

Affiliations

first authorsco-authorsvia INSPIRE