Поиск :
Личный кабинет :
Электронный каталог: Allakhverdyan, V. A. - Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gig...
Allakhverdyan, V. A. - Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gig...

Статья
Автор: Allakhverdyan, V. A.
Physical Review D: Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gig...
б.г.
ISBN отсутствует
Автор: Allakhverdyan, V. A.
Physical Review D: Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gig...
б.г.
ISBN отсутствует
Статья
Allakhverdyan, V.A.
Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gigaton Volume Detector / V.A.Allakhverdyan, I.A.Belolaptikov, I.V.Borina, V.Y.Dik, T.V.Elzhov, N.S.Gorshkov, E.V.Khramov, M.M.Kolbin, K.V.Konischev, A.V.Korobchenko, M.V.Kruglov, D.V.Naumov, E.N.Pliskovsky, B.A.Shaybonov, A.E.Sirenko, A.G.Solovjev, M.N.Sorokovikov, V.I.Tretyak, B.B.Ulzutuev, Y.V.Yablokova, S.I.Zavyalov, D.Y.Zvezdov, [a.o.]. – Text : electronic // Physical Review D. – 2025. – Vol. 112, No. 8. – P. 083025. – URL: https://doi.org/10.1103/jlz3-26lw.
Various theoretical models predict cosmic neutrinos with multi-PeV energies. The recent detection of a ∼10&sup(17) eV neutrino in the KM3NeT experiment suggests that these energetic particles can be studied with present-day installations. Here, we present upper limits on the flux of astrophysical neutrinos with energies (10&sup(15.5)–10&sup(20)) eV obtained with the largest liquid-water neutrino telescope, the Baikal Gigaton Volume Detector (GVD), operation using cascadelike events. We discuss astrophysical implications of these results and constrain several cosmogenic neutrino scenarios using a combination of Baikal-GVD, KM3NeT, IceCube, and Auger data.
Allakhverdyan, V.A.
Constraints on the Diffuse Flux of Multi-PeV Astrophysical Neutrinos Obtained with the Baikal Gigaton Volume Detector / V.A.Allakhverdyan, I.A.Belolaptikov, I.V.Borina, V.Y.Dik, T.V.Elzhov, N.S.Gorshkov, E.V.Khramov, M.M.Kolbin, K.V.Konischev, A.V.Korobchenko, M.V.Kruglov, D.V.Naumov, E.N.Pliskovsky, B.A.Shaybonov, A.E.Sirenko, A.G.Solovjev, M.N.Sorokovikov, V.I.Tretyak, B.B.Ulzutuev, Y.V.Yablokova, S.I.Zavyalov, D.Y.Zvezdov, [a.o.]. – Text : electronic // Physical Review D. – 2025. – Vol. 112, No. 8. – P. 083025. – URL: https://doi.org/10.1103/jlz3-26lw.
Various theoretical models predict cosmic neutrinos with multi-PeV energies. The recent detection of a ∼10&sup(17) eV neutrino in the KM3NeT experiment suggests that these energetic particles can be studied with present-day installations. Here, we present upper limits on the flux of astrophysical neutrinos with energies (10&sup(15.5)–10&sup(20)) eV obtained with the largest liquid-water neutrino telescope, the Baikal Gigaton Volume Detector (GVD), operation using cascadelike events. We discuss astrophysical implications of these results and constrain several cosmogenic neutrino scenarios using a combination of Baikal-GVD, KM3NeT, IceCube, and Auger data.
На полку