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arxiv: 1711.06520 · v3 · pith:O6X7OQTInew · submitted 2017-11-17 · 🌌 astro-ph.HE · hep-ph· nucl-th

Reaction rates and transport in neutron stars

classification 🌌 astro-ph.HE hep-phnucl-th
keywords neutronstarstransportratesreactioncorecrustdense
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Understanding signals from neutron stars requires knowledge about the transport inside the star. We review the transport properties and the underlying reaction rates of dense hadronic and quark matter in the crust and the core of neutron stars and point out open problems and future directions.

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Cited by 1 Pith paper

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.