http://arxiv.org/abs/2211.09447
We report on the first observation of the diffuse cosmic neutrino flux with the Baikal-GVD neutrino telescope. Using cascade-like events collected by Baikal-GVD in 2018–2021, a significant excess of events over the expected atmospheric background is observed. This excess is consistent with the high-energy diffuse cosmic neutrino flux observed by IceCube. The null cosmic flux assumption is rejected with a significance of 3.05$\sigma$. Assuming a single power law model of the astrophysical neutrino flux with identical contribution from each neutrino flavor, the following best-fit parameter values are found: the spectral index $\gamma_{astro}$ = $2.58^{+0.27}{-0.33}$ and the flux normalization $\phi{astro}$ = 3.04$^{+1.52}_{-1.21}$ per one flavor at 100 TeV.
B. Collaboration, V. Allakhverdyan, A. Avrorin, et. al.
Fri, 18 Nov 22
56/70
Comments: 9 pages; 5 figures; 2 tables
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