Journal article Open Access

VIP-2 —High-Sensitivity Tests on the Pauli Exclusion Principle for Electrons

Piscicchia, Kristian; Marton, Johann; Bartalucci, Sergio; Bazzi, Massimiliano; Bertolucci, Sergio; Bragadireanu, Mario; Cargnelli, Michael; Clozza, Alberto; Del Grande, Raffaele; De Paolis, Luca; Fiorini, Carlo; Guaraldo, Carlo; Iliescu, Mihail; Laubenstein, Matthias; Miliucci, Marco; Milotti, Edoardo; Napolitano, Fabrizio; Pichler, Andreas; Scordo, Alessandro; Shi, Hexi; Sirghi, Diana Laura; Sirghi, Florin; Sperandio, Laura; Vazquez Doce, Oton; Zmeskal, Johann; Curceanu, Catalina


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="URL">https://www.openaccessrepository.it/record/73490</identifier>
  <creators>
    <creator>
      <creatorName>Piscicchia, Kristian</creatorName>
      <givenName>Kristian</givenName>
      <familyName>Piscicchia</familyName>
      <affiliation>Centro Ricerche Enrico Fermi — Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Rome, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Marton, Johann</creatorName>
      <givenName>Johann</givenName>
      <familyName>Marton</familyName>
      <affiliation>Stefan Meyer Institute for Subatomic Physics, Kegelgasse 27, 1030 Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Bartalucci, Sergio</creatorName>
      <givenName>Sergio</givenName>
      <familyName>Bartalucci</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bazzi, Massimiliano</creatorName>
      <givenName>Massimiliano</givenName>
      <familyName>Bazzi</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bertolucci, Sergio</creatorName>
      <givenName>Sergio</givenName>
      <familyName>Bertolucci</familyName>
      <affiliation>Dipartimento di Fisica e Astronomia, University of Bologna and INFN—Sezione di Bologna, Via Irnerio 46, I-40126 Bologna, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bragadireanu, Mario</creatorName>
      <givenName>Mario</givenName>
      <familyName>Bragadireanu</familyName>
      <affiliation>Horia Hulubei National Institute of Physics and Nuclear Engineering, Str. Atomistilor No. 407, P.O. Box MG-6 Buchares-Magurele, Romania</affiliation>
    </creator>
    <creator>
      <creatorName>Cargnelli, Michael</creatorName>
      <givenName>Michael</givenName>
      <familyName>Cargnelli</familyName>
      <affiliation>Stefan Meyer Institute for Subatomic Physics, Kegelgasse 27, 1030 Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Clozza, Alberto</creatorName>
      <givenName>Alberto</givenName>
      <familyName>Clozza</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Del Grande, Raffaele</creatorName>
      <givenName>Raffaele</givenName>
      <familyName>Del Grande</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>De Paolis, Luca</creatorName>
      <givenName>Luca</givenName>
      <familyName>De Paolis</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Fiorini, Carlo</creatorName>
      <givenName>Carlo</givenName>
      <familyName>Fiorini</familyName>
      <affiliation>Politecnico di Milano, Dipartimento di Elettronica, Informazione e Bioingegneria and INFN Sezione di Milano, I-20133 Milano, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Guaraldo, Carlo</creatorName>
      <givenName>Carlo</givenName>
      <familyName>Guaraldo</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Iliescu, Mihail</creatorName>
      <givenName>Mihail</givenName>
      <familyName>Iliescu</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Laubenstein, Matthias</creatorName>
      <givenName>Matthias</givenName>
      <familyName>Laubenstein</familyName>
      <affiliation>INFN, Laboratori Nazionali del Gran Sasso, Via G. Acitelli 22, I-67100 L'Aquila, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Miliucci, Marco</creatorName>
      <givenName>Marco</givenName>
      <familyName>Miliucci</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Milotti, Edoardo</creatorName>
      <givenName>Edoardo</givenName>
      <familyName>Milotti</familyName>
      <affiliation>Dipartimento di Fisica, Università di Trieste and INFN—Sezione di Trieste, Via Valerio, 2, I-34127 Trieste, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Napolitano, Fabrizio</creatorName>
      <givenName>Fabrizio</givenName>
      <familyName>Napolitano</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Pichler, Andreas</creatorName>
      <givenName>Andreas</givenName>
      <familyName>Pichler</familyName>
      <affiliation>Stefan Meyer Institute for Subatomic Physics, Kegelgasse 27, 1030 Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Scordo, Alessandro</creatorName>
      <givenName>Alessandro</givenName>
      <familyName>Scordo</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Shi, Hexi</creatorName>
      <givenName>Hexi</givenName>
      <familyName>Shi</familyName>
      <affiliation>Stefan Meyer Institute for Subatomic Physics, Kegelgasse 27, 1030 Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Sirghi, Diana Laura</creatorName>
      <givenName>Diana Laura</givenName>
      <familyName>Sirghi</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Sirghi, Florin</creatorName>
      <givenName>Florin</givenName>
      <familyName>Sirghi</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Sperandio, Laura</creatorName>
      <givenName>Laura</givenName>
      <familyName>Sperandio</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Vazquez Doce, Oton</creatorName>
      <givenName>Oton</givenName>
      <familyName>Vazquez Doce</familyName>
      <affiliation>Excellence Cluster Universe, Technische Universität München, Boltzmannstraße 2, D-85748 Garching, Germany</affiliation>
    </creator>
    <creator>
      <creatorName>Zmeskal, Johann</creatorName>
      <givenName>Johann</givenName>
      <familyName>Zmeskal</familyName>
      <affiliation>Stefan Meyer Institute for Subatomic Physics, Kegelgasse 27, 1030 Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Curceanu, Catalina</creatorName>
      <givenName>Catalina</givenName>
      <familyName>Curceanu</familyName>
      <affiliation>INFN, Laboratori Nazionali di Frascati, Via E. Fermi 54, I-00044 Roma, Italy</affiliation>
    </creator>
  </creators>
  <titles>
    <title>VIP-2 —High-Sensitivity Tests on the Pauli Exclusion Principle for Electrons</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2020</publicationYear>
  <dates>
    <date dateType="Issued">2020-10-22</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/73490</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.3390/e22111195</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 sensitivity tests of the Pauli Exclusion Principle for electrons in the extremely low cosmic background environment of the underground Gran Sasso National Laboratory INFN (Italy). In particular, the VIP-2 Open Systems experiment was conceived to put strong constraints on those Pauli Exclusion Principle violation models which respect the so-called Messiah&amp;ndash;Greenberg superselection rule. The experimental technique consists of introducing a direct current in a copper conductor, and searching for the X-rays emission coming from a forbidden atomic transition from the L shell to the K shell of copper when the K shell is already occupied by two electrons. The analysis of the first three months of collected data (in 2018) is presented. The obtained result represents the best bound on the Pauli Exclusion Principle violation probability which fulfills the Messiah&amp;ndash;Greenberg rule.&lt;/p&gt;</description>
  </descriptions>
</resource>
158
41
views
downloads
Views 158
Downloads 41
Data volume 47.2 MB
Unique views 116
Unique downloads 36

Share

Cite as