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          <dc:title xml:lang="en">Simplified method to include the tensor contribution in α-cluster model</dc:title>
          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">Itagaki, N</jpcoar:creatorName>
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          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">Masui, H</jpcoar:creatorName>
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          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">Ito, M</jpcoar:creatorName>
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          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">Aoyama, S</jpcoar:creatorName>
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          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">Ikeda, K</jpcoar:creatorName>
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          <datacite:description descriptionType="Abstract">We propose a simplified model to directly take into account the contribution of the tensor interaction (SMT) for light nuclei by extending the α-cluster model. In Be, the energy curvewith respect to the relative distance between the two He clusters suggests that the cluster structure persists even though the tensor interaction contributes strongly. In addition to SMT, a simplified method to take into account the strong spin-orbit contribution is introduced and the coupling effects of these two models is shown to be important in C, in contrast to Be.</datacite:description>
          <datacite:description descriptionType="Other">(c)2006 The American Physical Society</datacite:description>
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          <dc:publisher xml:lang="en">American Physical Society</dc:publisher>
          <datacite:date dateType="Issued">2006</datacite:date>
          <dc:language>eng</dc:language>
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            <jpcoar:relatedIdentifier identifierType="DOI">http://doi.org/10.1103/PhysRevC.73.034310</jpcoar:relatedIdentifier>
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          <jpcoar:sourceTitle>Physical Review C</jpcoar:sourceTitle>
          <jpcoar:volume>73</jpcoar:volume>
          <jpcoar:pageStart>034310-1</jpcoar:pageStart>
          <jpcoar:pageEnd>034310-7</jpcoar:pageEnd>
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            <datacite:date dateType="Available">2016-11-22</datacite:date>
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