September 1, 2014 Journal article Open Access

Guglielmetti, Alessandra

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/29785</identifier>
  <creators>
    <creator>
      <creatorName>Guglielmetti, Alessandra</creatorName>
      <givenName>Alessandra</givenName>
      <familyName>Guglielmetti</familyName>
    </creator>
  </creators>
  <titles>
    <title>Nuclear astrophysics and underground accelerators</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2014</publicationYear>
  <dates>
    <date dateType="Issued">2014-09-01</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/29785</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1016/j.dark.2014.05.004</relatedIdentifier>
    <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">&lt;p&gt;Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it&lt;br&gt;
is important for understanding the energy generation, neutrino production and the synthesis of the&lt;br&gt;
elements in stars. Cross-section measurements are mainly hampered by the very low counting rate&lt;br&gt;
and cosmic background. An underground location is extremely advantageous for such studies, as&lt;br&gt;
demonstrated by the LUNA experiment in the Gran Sasso Laboratory (Italy). This paper reports on the&lt;br&gt;
results recently obtained by such an experiment and on the future perspectives in this field.&lt;/p&gt;</description>
  </descriptions>
</resource>