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Energy Transfer by Feebly Interacting Particles in Supernovae: The Trapping Regime

Damiano F. G. Fiorillo ^1,*, Tetyana Pitik ^2,3,†, and Edoardo Vitagliano ^4,5,‡

¹Deutsches Elektronen-Synchrotron DESY, Platanenallee 6, 15738 Zeuthen, Germany
²Department of Physics, University of California, Berkeley, Berkeley, California 94720, USA
³Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, Pennsylvania 16802, USA
⁴Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy
⁵Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy

^*Contact author: damianofg@gmail.com
^†Contact author: tetyana.pitik@berkeley.edu
^‡Contact author: edoardo.vitagliano@unipd.it

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Articles Citing

Energy Transfer by Feebly Interacting Particles in Supernovae: The Trapping Regime

Translating current ALP photon coupling strength bounds to the Randall-Sundrum model

Sub-GeV right-handed neutrino as a probe of neutrino mass generation in the minimal left-right symmetric model

Small Progenitors, Large Couplings: Type Ic Supernova Constraints on Radiatively Decaying Particles

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New constraints on axions with gamma-ray observations of the Crab Nebula

Exploring the dark axion portal in the LUXE-NPOD experiment

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Heavy dark photon handbook: Cosmological and astrophysical bounds

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Axions at the meV crossroads: theory, cosmology, astrophysics, and experiments

Spontaneous baryogenesis from axions on induced electroweak walls

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