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Palumbo, A.; Tan, W. P.; Goerres, J.; Wiescher, M.; Ozkan, N.; Guray, R. T.; Yalcin, C.
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>Palumbo, A.</dc:creator> <dc:creator>Tan, W. P.</dc:creator> <dc:creator>Goerres, J.</dc:creator> <dc:creator>Wiescher, M.</dc:creator> <dc:creator>Ozkan, N.</dc:creator> <dc:creator>Guray, R. T.</dc:creator> <dc:creator>Yalcin, C.</dc:creator> <dc:date>2012-01-01</dc:date> <dc:description>The statistical Hauser-Feshbach (HF) model performs poorly in calculating the (gamma, alpha) rates that are critical to the p process. Experimental work on elastic scattering of the tellurium isotopic chain [A. Palumbo et al. (unpublished)] provided a new parametrization of the alpha-optical potential and consequently new HF calculations of the (alpha, x) cross sections on Te120-130. However, reliable experimental cross sections of these isotopes have not been measured at energies relevant to the p process. To test the reliability of the HF calculations, we measured the (alpha, n) cross sections on Te-120, one of the p nuclei, using the activation technique. The results are compared with the HF model calculations.</dc:description> <dc:identifier>https://aperta.ulakbim.gov.trrecord/89015</dc:identifier> <dc:identifier>oai:zenodo.org:89015</dc:identifier> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights> <dc:source>PHYSICAL REVIEW C 85(2)</dc:source> <dc:title>Measurement of Te-120(alpha,n) cross sections relevant to the astrophysical p process</dc:title> <dc:type>info:eu-repo/semantics/article</dc:type> <dc:type>publication-article</dc:type> </oai_dc:dc>
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