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BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics

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arxiv 2405.09648 v1 pith:FDY56LAL submitted 2024-05-15 nucl-th hep-ph

classification nucl-thhep-ph
keywords particleschargeshydrodynamicsiccingidentifiedparticleccakecharge
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

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). In this study, we present a new 2+1 relativistic viscous hydrodynamic code called CCAKE which uses the Smoothed Particle Hydrodynamics (SPH) formalism to locally conserve BSQ charges, together with an extended description of the multi-dimensional equation of state (EoS) obtained from lattice Quantum Chromodynamics. Initial conditions for CCAKE are supplied by the ICCING model, which samples gluon splittings into quark anti-quark pairs to generate the initial BSQ charge distributions. We study correlations between the BSQ charges and find that local BSQ fluctuations remain finite during the evolution, with corresponding chemical potentials of ($\sim100$--$200 \,\rm MeV$) at freeze-out. We find that our framework produces reasonable multiplicities of identified particles and that ICCING has no significant effect on the collective flow of all charged particles nor of identified particles when only one particle of interest is considered. However, we show specifically for Pb+Pb collisions at the LHC $\sqrt{s_{NN}}=5.02$ TeV that ICCING does have an effect on collective flow of identified particles if two particles of interest are considered.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Initial-State Charge Density Predicts Final-State Net Charge Flow in Heavy-Ion Collisions

    nucl-th 2025-05 conditional novelty 6.0 of 10

    Initial baryon density, through a charge-odd cumulant estimator with a fitted coupling, predicts final net-proton elliptic flow in event-by-event hydrodynamic simulations.

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    nucl-th 2025-02 conditional novelty 6.0 of 10

    A new open-source calculation engine produces crust-to-core neutron star equations of state and shows that smooth matching choices change predicted radii and masses by several percent.

  3. An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars

    nucl-th 2025-05 conditional novelty 4.0 of 10

    Matching the crust and core equations of state with different smooth interpolation functions has only a modest effect on the predicted mass, radius, and tidal deformability of neutron stars, provided the matching occu...

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