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Bulk viscosity of two-color superconducting quark matter in neutron star mergers

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arxiv 2407.12493 v2 pith:3W4UKU3Y submitted 2024-07-17 nucl-th astro-ph.HEhep-ph

Bulk viscosity of two-color superconducting quark matter in neutron star mergers

classification nucl-th astro-ph.HEhep-ph
keywords quarkmatterbulkquarksviscositybluecolordamping
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the bulk viscosity of moderately hot and dense, neutrino-transparent color superconducting quark matter arising from weak-interaction-driven direct URCA processes. The quark matter is modeled using the Nambu--Jona-Lasinio model improved to account for vector and 't Hooft interactions as well as antisymmetric pairing among the red/green up and down quarks. The unpaired excitations are the strange quarks and the blue up or down quarks. We compute the relaxation rates associated with $d$ and $s$-quark decay and electron capture processes on $u$ quark for blue color. The resulting bulk viscosity for density oscillations in the 1--10\,kHz range shows a resonant peak at $T\sim 5\,\MeV$, and the damping time may drop below 10 ms. This is short enough to affect the postmerger evolution and is very similar to the damping predicted in nuclear matter.

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Cited by 2 Pith papers

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

  1. Bulk viscosity from neutron decays to dark baryons in neutron star matter

    astro-ph.HE 2025-09 conditional novelty 5.0

    Neutron dark decays modify the equation of state and either mildly suppress or strongly enhance bulk viscosity in neutron star merger conditions, depending on the in-medium decay rate.

  2. Nuclear matter equation of state and astrophysics

    nucl-th 2026-07 conditional

    A review of multimessenger constraints on the neutron-star equation of state, arguing composition remains undetermined and advocating a multidimensional EoS framework and the author-affiliated MUSES software.