January 1, 1999 Book section Open Access

M. Spinelli

DataCite XML Export

<?xml version='1.0' encoding='utf-8'?>
<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd">
  <identifier identifierType="DOI">10.15161/oar.it/1447936458.18</identifier>
  <creators>
    <creator>
      <creatorName>M. Spinelli</creatorName>
    </creator>
  </creators>
  <titles>
    <title>Atmoshperic Neutrino Oscillation Results  with  MACRO at Gran Sasso Laboraratory</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>1999</publicationYear>
  <subjects>
    <subject>96.40.Tv</subject>
    <subject>LNF - 99 / 014(P)</subject>
    <subject>Internal Note</subject>
    <subject>Nota Interna</subject>
  </subjects>
  <dates>
    <date dateType="Issued">1999-01-01</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Book section</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/17982</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://www.openaccessrepository.it/communities/infn</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by-nc-nd/4.0/">Creative Commons Attribution-NonCommercial-NoDerivatives</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">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.</description>
    <description descriptionType="Other">Presented at the VIII Internationl Workshp on Neutrino Telescopes 23-26 February, 1999, Campo S. Stefano, Venice (Italy)</description>
  </descriptions>
</resource>