E-viri
Recenzirano
Odprti dostop
-
Ackermann, M.; Ahrens, M.; Ansseau, I.; Axani, S.; Bai, X.; Bay, R.; BenZvi, S.; Bernardini, E.; Bourbeau, J.; Burgman, A.; Collin, G. H.; Correa, P.; Cross, R.; Dave, P.; Diaz, A.; Dujmovic, H.; Ehrhardt, T.; Eller, P.; Evans, J.; Fiedlschuster, S.; Friedman, E.; Fritz, A.; Goldschmidt, A.; Goswami, S.; Grégoire, T.; Griswold, S.; Halve, L.; Hauser, S.; Hickford, S.; Hill, G. C.; Huber, T.; Hultqvist, K.; Ishihara, A.; Jansson, M.; Kang, W.; Karg, T.; Karl, M.; Kellermann, M.; Kim, J.; Kiryluk, J.; Klein, S. R.; Kopper, C.; Koskinen, D. J.; Koundal, P.; Kovacevich, M.; Kowalski, M.; Larson, M. J.; Leonard, K.; Lyu, Y.; Mallik, P.; Mancina, S.; Meagher, K.; Medina, A.; Meier, M.; Meighen-Berger, S.; Merz, J.; Momenté, G.; Moulai, M.; Naab, R.; Nagai, R.; Neer, G.; Nygren, D. R.; Przybylski, G. T.; Raissi, A.; Rameez, M.; Rea, I. C.; Renschler, M.; Renzi, G.; Ruhe, T.; Santander, M.; Sarkar, S.; Schaufel, M.; Schmidt, T.; Schneider, J.; Seckel, D.; Shefali, S.; Smithers, B.; Snihur, R.; Spiczak, G. M.; Spiering, C.; Stettner, J.; Steuer, A.; Stokstad, R. G.; Stuttard, T.; Sullivan, G. W.; Tollefson, K.; Tomankova, L.; Trettin, A.; Tselengidou, M.; Tung, C. F.; Turcati, A.; Turcotte, R.; Turley, C. F.; Twagirayezu, J. P.; Unland Elorrieta, M. A.; Vandenbroucke, J.; Walck, C.; Weiss, M. J.; Werthebach, J.; Weyrauch, M.
Physical review. D, 07/2021, Letnik: 104, Številka: 2Journal Article
The IceCube Neutrino Observatory has established the existence of a high-energy all-sky neutrino flux of astrophysical origin. This discovery was made using events interacting within a fiducial region of the detector surrounded by an active veto and with reconstructed energy above 60 TeV, commonly known as the high-energy starting event sample (HESE). We revisit the analysis of the HESE sample with an additional 4.5 years of data, newer glacial ice models, and improved systematics treatment. This paper describes the sample in detail, reports on the latest astrophysical neutrino flux measurements, and presents a source search for astrophysical neutrinos. We give the compatibility of these observations with specific isotropic flux models proposed in the literature as well as generic power-law-like scenarios. Assuming νe: νμ: ντ= 1 : 1 : 1 , and an equal flux of neutrinos and antineutrinos, we find that the astrophysical neutrino spectrum is compatible with an unbroken power law, with a preferred spectral index of 2.87−0.19+0.20 for the 68% confidence interval.
Avtor
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.