Shock Breakouts from Compact Circumstellar Medium Surrounding Core-collapse Supernova Progenitors May Contribute Significantly to the Observed ≳10 TeV Neutrino Background

Growing observational evidence suggests that enhanced mass loss from the progenitors of core-collapse supernovae (SNe) is common during  ~1 yr preceding the explosion, creating an optically thick circumstellar medium (CSM) shell at  ~10 ^14.5 cm radii. We show that if such mass loss is indeed common...

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Detaylı Bibliyografya

Asıl Yazarlar:	Eli Waxman, Tal Wasserman, Eran O. Ofek, Avishay Gal-Yam
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	IOP Publishing 2025-01-01
Seri Bilgileri:	The Astrophysical Journal
Konular:	Neutrino astronomy High energy astrophysics Supernovae
Online Erişim:	https://doi.org/10.3847/1538-4357/ad9a6b
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