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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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Detalles Bibliográficos
Autores principales:	Buccheri, M., Cosentino, S. P., Pumo, M. L.
Formato:	Preprint
Publicado:	2026
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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