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High-energy neutrino flux from SN2024ggi: constraints from semi-analytic modeling of its post-explosive emission

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Buccheri, M., Cosentino, S. P., Pumo, M. L.
Format:	Preprint
Publié:	2026
Sujets:	High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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