The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux

By I. C. M. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson and 310 more. 2016

220 citations recorded by the source corpus.

The recent discovery of a diffuse cosmic neutrino flux extending up to PeV energies raises the question of which astrophysical sources generate this signal. One class of extragalactic sources which may produce such high-energy neutrinos are blazars. We present a likelihood analysis searching for cumulative neutrino emission from blazars in the 2nd Fermi-LAT AGN catalogue (2LAC) using an IceCube neutrino dataset 2009-12 which was optimised for the detection of individual sources. In contrast to previous searches with IceCube, the populations investigated contain up to hundreds of sources, the largest one being the entire blazar sample in the 2LAC catalogue. No significant excess is observed and upper limits for the cumulative flux from these populations are obtained. These constrain the maximum contribution of the 2LAC blazars to the observed astrophysical neutrino flux to be $27 \%$ or less between around 10 TeV and 2 PeV, assuming equipartition of flavours at Earth and a single power-law spectrum with a spectral index of $-2.5$. We can still exclude that the 2LAC blazars (and sub-populations) emit more than $50 \%$ of the observed neutrinos up to a spectral index as hard as $-2.2$ in the same energy range. Our result takes into account that the neutrino source count distribution is unknown, and it does not assume strict proportionality of the neutrino flux to the measured 2LAC $\gamma$-ray signal for each source. Additionally, we constrain recent models for neutrino emission by blazars.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/42cd08d23f9fa495ad6a095dc17818c94f9ce4cb

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Citations in the corpus

• Blazar Flares as an Origin of High-energy Cosmic Neutrinos? (2018, methodology): “…blazar contribution to the INB has been constrained by different types of analyses: (i) diffuse searches for extremely high-energy (EHE) neutrinos (Aartsen et al. 2016, 2017a), (ii) event clustering and auto-correlation analyses (Murase & Waxman 2016; Aartsen et al. 2015, 2017b), and (iii)…”