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Possible $ν$ Source Class: 3-sigma Detection of High-Energy Neutrinos from Supermassive Black Hole Binary Candidates

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	D, Pugazhendhi A, Bouri, Subhadip, Zhou, Bei, Rachana, Laha, Ranjan
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment High Energy Physics - Phenomenology
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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