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Expected impact from weak reactions with light nuclei in core-collapse supernova simulations

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arxiv 1512.00193 v1 pith:4GSIE4NG submitted 2015-12-01 astro-ph.HE nucl-th

Expected impact from weak reactions with light nuclei in core-collapse supernova simulations

T. Fischer , G. Mart\'inez-Pinedo , M. Hempel , L. Huther , G. R\"opke , S. Typel , A. Lohs This is my paper
classification astro-ph.HE nucl-th
keywords lightclusterscore-collapseduringexplosionimpactonsetpossible
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the role of light nuclear clusters in simulations of core-collapse supernovae. Expressions for the reaction rates are developed for a large selection of charged current absorption and scattering processes with light clusters. Medium modifications are taken into account at the mean-field level. We explore the possible impact on the supernova dynamics and the neutrino signal during the mass accretion phase prior to the possible explosion onset as well as during the subsequent protoneutron star deleptnoization after the explosion onset has been launched.

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  1. Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae

    nucl-th 2026-04 unverdicted novelty 6.0

    Including multineutron states in supernova equations of state reduces unbound neutron fractions, raises proton chemical potentials, promotes heavier nuclei, and lowers overall free energy in neutron-rich conditions.