Journal article Open Access

An excited state of Th 229 at 3.5 eV

Helmer, R. G.; Reich, C. W.


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  <identifier identifierType="URL">https://zenodo.org/record/1233767</identifier>
  <creators>
    <creator>
      <creatorName>Helmer, R. G.</creatorName>
      <givenName>R. G.</givenName>
      <familyName>Helmer</familyName>
    </creator>
    <creator>
      <creatorName>Reich, C. W.</creatorName>
      <givenName>C. W.</givenName>
      <familyName>Reich</familyName>
    </creator>
  </creators>
  <titles>
    <title>An excited state of Th 229 at 3.5 eV</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>1994</publicationYear>
  <dates>
    <date dateType="Issued">1994-04-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/1233767</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/physrevc.49.1845</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/publicdomain/zero/1.0/legalcode">Creative Commons Zero v1.0 Universal</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">It has been known for many years that the first excited state of Th229 lies close to the ground state. Originally this energy was given as &amp;lt;0.1 keV; later, the authors reported a value of -1±4 eV. In an attempt to improve the value for this level energy, we have remeasured the energies of a number of γ rays from U223 whose positions in the Th229 level scheme can be used to establish it. Compared with our earlier study, we have considered more γ rays in Th229, used more well-measured energy calibration and reference lines, used more detectors, used detectors with better low-energy resolution, more closely matched the counting rates in the γ-ray peaks whose relative energy is measured, and specifically considered certain systematic errors. More than 111 γ-ray spectra have been measured. From this large set of measurements we have deduced a value of 3.5±1.0 eV for the energy of this level.</description>
  </descriptions>
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