Diffuse neutrinos from extragalactic supernova remnants: Dominating the 100 TeV IceCube flux
IceCube has measured a diffuse astrophysical flux of TeV–PeV neutrinos. The most plausible sources are unique high energy cosmic ray accelerators like hypernova remnants (HNRs) and remnants from gamma ray bursts in star-burst galaxies, which can produce primary cosmic rays with the required energies...
Main Authors: | Sovan Chakraborty, Ignacio Izaguirre |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2015-05-01
|
Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269315002750 |
Similar Items
-
The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova
Searches, Ice Properties
by: Collaboration, TI
Published: (2011) -
The IceCube Neutrino Observatory Part V: Neutrino Oscillations and
Supernova Searches
by: Collaboration, I, et al.
Published: (2013) -
IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae
by: Collaboration, I, et al.
Published: (2011) -
Constraining High-energy Neutrino Emission from Supernovae with IceCube
by: R. Abbasi, et al.
Published: (2023-01-01) -
IceCube sensitivity for low-energy neutrinos from nearby supernovae (Corrigendum)
by: IceCube Collaboration
Published: (2014)