Book section Open Access
M. Spinelli
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>M. Spinelli</dc:creator> <dc:date>1999-01-01</dc:date> <dc:description>We present updated results of the measurement of the atmospheric neutrino flux with the MACRO detector at Gran Sasso, using three data sets spread in a large energy range. In the high energy range, the upgoing throughgoing muon data set is in favor of νμ →ντ oscillation hypothesis with a probability of 36.6% against the 0.36% for the no oscillation hypothesis.In the low energy range, the two data set are also in favor to the oscillation hypothesis showing a large defict for IU events and a reduced defict for US+ID events, since only the US events ( |50% ) are expected to oscillate Assuming a νμ →ντ oscillation scheme, the results suggest a large range of the parameter values centered around Dm2=0.0025 eV2, sin2 2q = 1.</dc:description> <dc:identifier>https://www.openaccessrepository.it/record/17982</dc:identifier> <dc:identifier>10.15161/oar.it/1447936458.18</dc:identifier> <dc:language>eng</dc:language> <dc:relation>url:https://www.openaccessrepository.it/communities/infn</dc:relation> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>https://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights> <dc:subject>96.40.Tv</dc:subject> <dc:subject>LNF - 99 / 014(P)</dc:subject> <dc:subject>Internal Note</dc:subject> <dc:subject>Nota Interna</dc:subject> <dc:title>Atmoshperic Neutrino Oscillation Results with MACRO at Gran Sasso Laboraratory</dc:title> <dc:type>info:eu-repo/semantics/bookPart</dc:type> <dc:type>publication-section</dc:type> </oai_dc:dc>
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