• Corpus ID: 255372292

Bump-hunting in the diffuse flux of high-energy cosmic neutrinos

  title={Bump-hunting in the diffuse flux of high-energy cosmic neutrinos},
  author={Damano F. G. Fiorillo and Mauricio Bustamante},

Figures and Tables from this paper



High-energy neutrinos from active galactic nuclei.

The spectrum and high-energy ν background flux are calculated from photomeson production in active galactic nuclei using data from the Large Hadron Collider.

Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube

Inelasticity, the fraction of a neutrino's energy transferred to hadrons, is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV energies with Ic

High-energy neutrinos from photomeson processes in blazars.

It is predicted that km(2) neutrino telescopes will > or similar to 1 neutrinos per year from flat spectrum radio quasars such as 3C 279.

Diffuse fluxes of cosmic high-energy neutrinos

Production spectra of high-energy neutrinos from galactic cosmic-ray interactions with interstellar gas and extragalactic ultrahigh-energy cosmic-ray interactions with microwave blackbody photons are

Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino.

The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an

Bayesian constraints on the astrophysical neutrino source population from IceCube data

We present constraints on an astrophysical population of neutrino sources imposed by recent data from the IceCube neutrino observatory. By using the IceCube point source search method to model the ...

Inferring the Flavor of High-Energy Astrophysical Neutrinos at Their Sources.

A Bayesian method is introduced that infers the flavor composition at the neutrino sources based on the flavour composition measured at Earth, and finds that the present data from the IceCube neutrinos telescope favor neutRino production via the decay of high-energy pions and rule out production viaThe decay of neutrons.