E-resources
-
Aartsen, M. G.; Ackermann, M.; Ahlers, M.; Altmann, D.; Anderson, T.; Bay, R.; BenZvi, S.; Bernardini, E.; Besson, D. Z.; Binder, G.; Bindig, D.; Blaufuss, E.; Bohm, C.; Böser, S.; Botner, O.; Brayeur, L.; Cowen, D. F.; Davis, J. C.; de André, J. P. A. M.; Dembinski, H.; de Wasseige, G.; Eagan, R.; Eberhardt, B.; Ehrhardt, T.; Eichmann, B.; Euler, S.; Evenson, P. A.; Fedynitch, A.; Feintzeig, J.; Felde, J.; Finley, C.; Flis, S.; Gaisser, T. K.; Gladstone, L.; Golup, G.; Gonzalez, J. G.; Hallgren, A.; Halzen, F.; Helbing, K.; Hellauer, R.; Hignight, J.; Hoffmann, R.; Hultqvist, K.; In, S.; Karg, T.; Karle, A.; Keivani, A.; Kiryluk, J.; Kohnen, G.; Koirala, R.; Kolanoski, H.; Kurahashi, N.; Lanfranchi, J. L.; Lesiak-Bzdak, M.; Leuermann, M.; Lu, L.; Madsen, J.; Maggi, G.; McNally, F.; Meagher, K.; Medici, M.; Meli, A.; Meures, T.; Morse, R.; Naumann, U.; Neer, G.; Obertacke, A.; Omairat, A.; Pinat, E.; Posselt, J.; Price, P. B.; Pütz, J.; Relich, M.; Resconi, E.; Rhode, W.; Rongen, M.; Rott, C.; Ruhe, T.; Sandrock, A.; Schmidt, T.; Seckel, D.; Stanev, T.; Stezelberger, T.; Stößl, A.; Terliuk, A.; Tobin, M. N.; Tosi, D.; Unger, E.; Vandenbroucke, J.; Vanheule, S.; Veenkamp, J.; Vraeghe, M.; Wallace, A.; Wandkowsky, N.; Weaver, Ch; Wendt, C.; Whelan, B. J.; Wiebe, K.; Wille, L.; Wood, T. R.
Physical review. D, 01/2016, Volume: 93, Issue: 2Journal Article
The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7sigma significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event-one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches.
Author
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Shelf entry
Permalink
- URL:
Impact factor
Access to the JCR database is permitted only to users from Slovenia. Your current IP address is not on the list of IP addresses with access permission, and authentication with the relevant AAI accout is required.
Year | Impact factor | Edition | Category | Classification | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Select the library membership card:
If the library membership card is not in the list,
add a new one.
DRS, in which the journal is indexed
Database name | Field | Year |
---|
Links to authors' personal bibliographies | Links to information on researchers in the SICRIS system |
---|
Source: Personal bibliographies
and: SICRIS
The material is available in full text. If you wish to order the material anyway, click the Continue button.