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Muonization of supernova matter

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arxiv 2008.13628 v2 pith:5PCKT5CF submitted 2020-08-31 astro-ph.HE

Tobias Fischer , Gang Guo , Gabriel Martínez-Pinedo , Matthias Liebendörder , Anthony Mezzacappa This is my paper · ORCID
classification astro-ph.HE
keywords muonsbolligcore-collapseemissionmuonneutrinoneutrinosonly
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The present article investigates the impact of muons on core-collapse supernovae, with particular focus on the early muon neutrino emission. While the presence of muons is well understood in the context of neutron stars, until the recent study by Bollig et al. [Phys. Rev. Lett. 119, 242702 (2017)] the role of muons in core-collapse supernovae had been neglected--electrons and neutrinos were the only leptons considered. In their study, Bollig et al. disentangled the muon and tau neutrinos and antineutrinos and included a variety of muonic weak reactions, all of which the present paper follows closely. Only then does it becomes possible to quantify the appearance of muons shortly before stellar core bounce and how the post-bounce prompt neutrino emission is modified

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Cited by 3 Pith papers

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    Collisional neutrino flavor instabilities settle into a state at the edge of instability with nonzero flavor coherence, and explicit formulas predict this final state.

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    hep-ph 2026-07 conditional novelty 6.0 of 10

    Orbital timing of the Hulse-Taylor binary pulsar gives the strongest published limits on quadratic axion-muon couplings for axion masses below about 10^-12 eV, and complementary limits on axion-neutron and axion-elect...

  3. Strongly interacting matter with criticality induced by modified excluded volume in core-collapse supernova simulations

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    Modified-excluded-volume EOS with continuous van der Waals phase transition yields CCSN explosions and a several-millisecond neutrino burst, while the same EOS under Gibbs construction fails to explode.

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