dc.creatorMoura C.
dc.date2006
dc.date2015-06-30T18:01:06Z
dc.date2015-11-26T14:14:19Z
dc.date2015-06-30T18:01:06Z
dc.date2015-11-26T14:14:19Z
dc.date.accessioned2018-03-28T21:15:11Z
dc.date.available2018-03-28T21:15:11Z
dc.identifier0735403007; 9780735403000
dc.identifierAip Conference Proceedings. , v. 809, n. , p. 190 - 192, 2006.
dc.identifier0094243X
dc.identifier10.1063/1.2160982
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-33751248485&partnerID=40&md5=cd26e451c3d02fd9d1b906f70889a925
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/102690
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/102690
dc.identifier2-s2.0-33751248485
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1242510
dc.descriptionUltra-High Energy (UHE) neutrinos (ν's) coming from extra-galactic sources may arrive at the Earth's atmosphere in the same proportion for all the three ν flavor states. Using a Fluorescence Detector (FD) one may detect tau-neutrinos (ντ's) by searching for double Extensive Air Showers (EAS's) in the atmosphere, the so called Double-Bang (DB) events. This kind of events are very rare but can give some information about neutrino flux and cross section. © 2006 American Institute of Physics.
dc.description809
dc.description
dc.description190
dc.description192
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dc.languageen
dc.publisher
dc.relationAIP Conference Proceedings
dc.rightsaberto
dc.sourceScopus
dc.titleDetection Of Ultra-high Energy Tau-neutrino By Double-bang Event
dc.typeActas de congresos


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