2026/08/06 by The KM3NeT Collaboration
Physics and Astronomy · #astro-ph.HE #hep-ex
33 pages, 24 figures
arxiv created 2026/08/06 · arxiv updated 2026/08/07
We report on the search performed for a diffuse astrophysical neutrino flux from the full sky and from a specific region of the Galactic plane, the Galactic Ridge. The study uses the dataset collected with the first KM3NeT/ARCA configurations with 6, 8, 19, and 21 active detection units, corresponding to a total livetime of 640 days. For the all-sky analysis, the fitted single-flavour astrophysical neutrino flux parameters, under the single power-law assumption, are ϕ01f = 3.0+2.1-2.0 × 10-18 GeV-1 cm-2 s-1 sr-1 with spectral index γ= 3.00+0.30-0.35 at 68% credible level. The Galactic Ridge fit does not yield constraints for the flux parameters with the current sensitivity. For both analyses upper limits are derived and compared with state-of-the-art measurements. While the analysis of these datasets has not yielded statistically significant results, the developed methods provide a solid basis for future measurements with the KM3NeT detector.