One-point fluctuation analysis of the high-energy neutrino sky

Research output: Contribution to journalJournal articlepeer-review

We perform the first one-point fluctuation analysis of the high-energy neutrino sky. This method reveals itself to be especially suited to contemporary neutrino data, as it allows to study the properties of the astrophysical components of the high-energy flux detected by the IceCube telescope, even with low statistics and in the absence of point source detection. Besides the veto-passing atmospheric foregrounds, we adopt a simple model of the high-energy neutrino background by assuming two main extra-galactic components: star-forming galaxies and blazars. By leveraging multi-wavelength data from Herschel and Fermi, we predict the spectral and anisotropic probability distributions for their expected neutrino counts in IceCube. We find that star-forming galaxies are likely to remain a diffuse background due to the poor angular resolution of IceCube, and we determine an upper limit on the number of shower events that can reasonably be associated to blazars. We also find that upper limits on the contribution of blazars to the measured flux are unfavourably affected by the skewness of the blazar flux distribution. One-point event clustering and likelihood analyses of the IceCube HESE data suggest that this method has the potential to dramatically improve over more conventional model-based analyses, especially for the next generation of neutrino telescopes.
Original languageEnglish
Article number057
JournalJournal of Cosmology and Astroparticle Physics
Volume2017
Issue number03
ISSN1475-7516
DOIs
Publication statusPublished - 29 Mar 2017

Bibliographical note

41 pages, 6 figures, 2 tables; different blazar model than v1 but same results

    Research areas

  • astro-ph.HE, astro-ph.IM, hep-ph

Links

ID: 184720290