Neutrinos diffusing through dense dark matter spikes around supermassive black holes can be delayed by days, but the accompanying flux suppression means dark matter alone probably cannot explain the observed 100+ day delays from tidal disruption events.
Detecting High-Energy Neutrinos from Galactic Supernovae with ATLAS
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
We show that ATLAS, a collider detector, can measure the flux of high-energy supernova neutrinos, which can be produced from days to months after the explosion. Using Monte Carlo simulations for predicted fluxes, we find at most $\mathcal{O}(0.1-1)$ starting events and $\mathcal{O}(10-100)$ throughgoing events from a supernova 10 kpc away. Possible Galactic supernovae from Betelgeuse and Eta Carinae are further analyzed as demonstrative examples. We argue that even with limited statistics, ATLAS has the ability to discriminate among flavors and between neutrinos and antineutrinos, making it an unique neutrino observatory so far unmatched in this capability.
citation-role summary
background 1
citation-polarity summary
fields
hep-ph 1years
2024 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Neutrino Diffusion within Dark Matter Spikes
Neutrinos diffusing through dense dark matter spikes around supermassive black holes can be delayed by days, but the accompanying flux suppression means dark matter alone probably cannot explain the observed 100+ day delays from tidal disruption events.