1 Ocak 2015 Dergi makalesi Açık Erişim

Yalcin, C.; Gyuerky, Gy.; Rauscher, T.; Kiss, G. G.; Ozkan, N.; Guray, R. T.; Halasz, Z.; Szuecs, T.; Fueloep, Zs.; Farkas, J.; Korkulu, Z.; Somorjai, E.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/81333</identifier>
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      <creatorName>Yalcin, C.</creatorName>
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      <creatorName>Gyuerky, Gy.</creatorName>
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      <affiliation>Inst Nucl Res MTA Atomki, H-4001 Debrecen, Hungary</affiliation>
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      <creatorName>Ozkan, N.</creatorName>
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      <creatorName>Guray, R. T.</creatorName>
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      <creatorName>Fueloep, Zs.</creatorName>
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      <creatorName>Farkas, J.</creatorName>
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      <creatorName>Korkulu, Z.</creatorName>
      <givenName>Z.</givenName>
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      <affiliation>Kocaeli Univ, Dept Phys, TR-41380 Umuttepe, Kocaeli, Turkey</affiliation>
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      <creatorName>Somorjai, E.</creatorName>
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      <affiliation>Inst Nucl Res MTA Atomki, H-4001 Debrecen, Hungary</affiliation>
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  <titles>
    <title>Test Of Statistical Model Cross Section Calculations For Alpha-Induced Reactions On Ag-107 At Energies Of Astrophysical Interest</title>
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  <publisher>Aperta</publisher>
  <publicationYear>2015</publicationYear>
  <dates>
    <date dateType="Issued">2015-01-01</date>
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  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/PhysRevC.91.034610</relatedIdentifier>
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  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
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  <descriptions>
    <description descriptionType="Abstract">Background: Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessary input to nuclear reaction network simulations for studying the origin of p nuclei. Past experiments have found a considerable difference between theoretical and experimental cross sections in some cases, especially for (alpha,gamma) reactions at low energy. Therefore, it is important to experimentally test theoretical cross section predictions at low, astrophysically relevant energies.</description>
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