dc.creator | Guzzo, MM | |
dc.creator | Moura, CA | |
dc.date | 2006 | |
dc.date | MAY | |
dc.date | 2014-11-15T11:12:39Z | |
dc.date | 2015-11-26T16:10:42Z | |
dc.date | 2014-11-15T11:12:39Z | |
dc.date | 2015-11-26T16:10:42Z | |
dc.date.accessioned | 2018-03-28T22:59:19Z | |
dc.date.available | 2018-03-28T22:59:19Z | |
dc.identifier | Astroparticle Physics. Elsevier Science Bv, v. 25, n. 4, n. 277, n. 283, 2006. | |
dc.identifier | 0927-6505 | |
dc.identifier | WOS:000237566700006 | |
dc.identifier | 10.1016/j.astropartphys.2006.03.002 | |
dc.identifier | http://www.repositorio.unicamp.br/jspui/handle/REPOSIP/76886 | |
dc.identifier | http://www.repositorio.unicamp.br/handle/REPOSIP/76886 | |
dc.identifier | http://repositorio.unicamp.br/jspui/handle/REPOSIP/76886 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/1266939 | |
dc.description | We investigate the possibility of detecting ultra-high energy cosmic tau-neutrinos by means of a process involving a double extensive air shower, the so-called double-bang phenomenon. In this process a primary tau-neutrino interacts with an atmospheric quark creating a hadronic extensive air shower that contains a tau which subsequently decays creating a second extensive air shower. The number of these events strongly depends on the cross section and on the flux of ultra-high energy tau-neutrinos arriving at the Earth's atmosphere. We estimate the potential of optical detectors to observe double-bang events induced by tau-neutrinos with energies of about 1 EeV whose detection may confirm the maximal mixing observed in the atmospheric neutrinos also for ultra-high energy neutrinos, and give information on the neutrino flux and cross-section. For neutrino-nucleon standard model extrapolated cross-section and thick source model of flux (MPR), we estimate an event rate of 0.48 y(-1) for an observatory with two fluorescence detectors with 90% efficiency in the neutrino energy range 0.5 < E-v < 5 EeV. (c) 2006 Elsevier B.V. All rights reserved. | |
dc.description | 25 | |
dc.description | 4 | |
dc.description | 277 | |
dc.description | 283 | |
dc.language | en | |
dc.publisher | Elsevier Science Bv | |
dc.publisher | Amsterdam | |
dc.publisher | Holanda | |
dc.relation | Astroparticle Physics | |
dc.relation | Astropart Phys. | |
dc.rights | fechado | |
dc.rights | http://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy | |
dc.source | Web of Science | |
dc.subject | UHECR | |
dc.subject | EAS | |
dc.subject | Tau-neutrinos | |
dc.subject | double-bang | |
dc.subject | Auger observatory | |
dc.subject | Topological Defects | |
dc.subject | Cosmic-rays | |
dc.subject | Oscillations | |
dc.subject | Spectrum | |
dc.subject | Showers | |
dc.title | Ultra high energy tau-neutrinos and fluorescence detectors: A phenomenological approach | |
dc.type | Artículos de revistas | |