October 31, 2019 Journal article Open Access

Piscicchia, K.; Pichler, A.; Amirkhani, A.; Bartalucci, S.; Bertolucci, S.; Bazzi, M.; Bragadireanu, M.; Cargnelli, M.; Clozza, A.; Del Grande, R.; De Paolis, L.; Egger, J.; Fiorini, C.; Guaraldo, C.; Iliescu, M.; Laubenstein, M.; Marton, J.; Miliucci, M.; Milotti, E.; Pietreanu, D.; Scordo, A.; Shi, H.; Sirghi, D. L.; Sirghi, F.; Sperandio, L.; Vazquez Doce, O.; Zmeskal, J.; Curceanu, C.

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      <affiliation>Centro Fermi — Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Rome, Italy; Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Amirkhani, A.</creatorName>
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      <affiliation>Politecnico di Milano, Dipartimento di Elettronica, Informazione e Bioingegneria and INFN Sezione di Milano, Milano, Italy</affiliation>
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      <creatorName>Bartalucci, S.</creatorName>
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      <creatorName>Bertolucci, S.</creatorName>
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      <affiliation>Dipartimento di Fisica e Astronomia, Università di Bologna, Italy</affiliation>
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      <creatorName>Bazzi, M.</creatorName>
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      <creatorName>Bragadireanu, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Bragadireanu</familyName>
      <affiliation>Institutul National de Fizica si Inginerie Nucleara — "Horia Hulubei" (IFIN-HH) Măgurele, Romania; Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Cargnelli, M.</creatorName>
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      <affiliation>Stefan-Meyer-Institute for Subatomic Physics Austrian Academy of Science, Austria</affiliation>
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      <creatorName>Clozza, A.</creatorName>
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      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Del Grande, R.</creatorName>
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      <familyName>Del Grande</familyName>
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      <creatorName>De Paolis, L.</creatorName>
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      <familyName>De Paolis</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Egger, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Egger</familyName>
      <affiliation>Institut de Physique, Université de Neuchâtel, Switzerland</affiliation>
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      <creatorName>Fiorini, C.</creatorName>
      <givenName>C.</givenName>
      <familyName>Fiorini</familyName>
      <affiliation>Politecnico di Milano, Dipartimento di Elettronica, Informazione e Bioingegneria and INFN Sezione di Milano, Milano, Italy</affiliation>
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      <creatorName>Guaraldo, C.</creatorName>
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      <familyName>Guaraldo</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Iliescu, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Iliescu</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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    <creator>
      <creatorName>Laubenstein, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Laubenstein</familyName>
      <affiliation>Laboratori Nazionali del Gran Sasso, INFN, Italy</affiliation>
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      <creatorName>Marton, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Marton</familyName>
      <affiliation>Stefan-Meyer-Institute for Subatomic Physics Austrian Academy of Science, Austria</affiliation>
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      <creatorName>Miliucci, M.</creatorName>
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      <familyName>Miliucci</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Milotti, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Milotti</familyName>
      <affiliation>Dipartimento di Fisica, Università di Trieste and INFN-Sezione di Trieste, Italy</affiliation>
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      <creatorName>Pietreanu, D.</creatorName>
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      <familyName>Pietreanu</familyName>
      <affiliation>Institutul National de Fizica si Inginerie Nucleara — "Horia Hulubei" (IFIN-HH) Măgurele, Romania; Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Scordo, A.</creatorName>
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      <familyName>Scordo</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
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      <creatorName>Shi, H.</creatorName>
      <givenName>H.</givenName>
      <familyName>Shi</familyName>
      <affiliation>Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, Austria</affiliation>
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      <creatorName>Sirghi, D. L.</creatorName>
      <givenName>D. L.</givenName>
      <familyName>Sirghi</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy; Institutul National de Fizica si Inginerie Nucleara — "Horia Hulubei" (IFIN-HH) Măgurele, Romania</affiliation>
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      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy; Institutul National de Fizica si Inginerie Nucleara — "Horia Hulubei" (IFIN-HH) Măgurele, Romania</affiliation>
    </creator>
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      <creatorName>Sperandio, L.</creatorName>
      <givenName>L.</givenName>
      <familyName>Sperandio</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Vazquez Doce, O.</creatorName>
      <givenName>O.</givenName>
      <familyName>Vazquez Doce</familyName>
      <affiliation>Excellence Cluster Universe, Technische Universität München, Germany</affiliation>
    </creator>
    <creator>
      <creatorName>Zmeskal, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Zmeskal</familyName>
      <affiliation>Stefan-Meyer-Institute for Subatomic Physics Austrian Academy of Science, Austria</affiliation>
    </creator>
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      <creatorName>Curceanu, C.</creatorName>
      <givenName>C.</givenName>
      <familyName>Curceanu</familyName>
      <affiliation>Laboratori Nazionali di Frascati, INFN, Italy; Centro Fermi — Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Rome, Italy; Institutul National de Fizica si Inginerie Nucleara — "Horia Hulubei" (IFIN-HH) Măgurele, Romania</affiliation>
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  <titles>
    <title>TESTING THE PAULI EXCLUSION PRINCIPLE IN THE COSMIC SILENCE</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-10-31</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/30676</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.5506/APhysPolB.51.97</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://www.openaccessrepository.it/communities/infn</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;The VIP Collaboration is performing high precision tests of the Pauli&amp;nbsp;Exclusion Principle for electrons in the extremely low cosmic background&amp;nbsp;environment of the Underground Gran Sasso Laboratories of INFN (Italy). The experimental technique consists in introducing a DC current in a copper conductor, searching for K&lt;span class="math-tex"&gt;\(_{\alpha}\)&lt;/span&gt;&amp;nbsp;PEP-forbidden atomic transitions when the K shell is already occupied by two electrons. VIP set an upper limit on&amp;nbsp;the PEP-violation probability &lt;span class="math-tex"&gt;\(\frac{1}{2} \beta^2 &amp;lt; 4.7 \times 10^{-29}\)&lt;/span&gt;. The aim of the upgraded VIP-2 experiment is to improve this result at least by two orders of magnitude. The improved experimental setup and the results of a preliminary&amp;nbsp;data analysis, corresponding to the the first run of the VIP-2 data taking (2016&amp;ndash;2017), will be presented.&lt;/p&gt;</description>
  </descriptions>
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