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Calculation of Gamma Strength Functions for Photonucleon Reactions

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dc.creator Mavi, B.
dc.creator AKKURT, İskender
dc.creator KARPUZ, NURDAN
dc.date 2015-07-31T21:00:00Z
dc.date.accessioned 2020-10-06T10:51:16Z
dc.date.available 2020-10-06T10:51:16Z
dc.identifier a4e5354a-85b3-4bfa-822e-26e6e709c5c6
dc.identifier 10.12693/aphyspola.128.b-414
dc.identifier https://avesis.sdu.edu.tr/publication/details/a4e5354a-85b3-4bfa-822e-26e6e709c5c6/oai
dc.identifier.uri http://acikerisim.sdu.edu.tr/xmlui/handle/123456789/68306
dc.description The cross section for (gamma,N) reaction is important for investigation of nuclear structure, especially in low-energy giant dipole resonance (GDR). The total cross sections of C-12(gamma, n)C-11 and C-12(gamma,p)B-11 reactions, calculated using TALYS 1.2 nuclear code, are 15.5 to 40 MeV and 15 to 110 MeV, respectively. In the calculations, the default pre-equilibrium models and Brink-Axel Lorentzian model in all of the gamma strength functions have been used. The effects of the gamma strength function on the cross section exchange data has determined the most compatible model type. The results are compared with the experimental data from the EXFOR database and the evaluated nuclear data from TENDL-2012. Our calculated results are in good agreement with the previously reported experimental results.
dc.language eng
dc.rights info:eu-repo/semantics/closedAccess
dc.title Calculation of Gamma Strength Functions for Photonucleon Reactions
dc.type info:eu-repo/semantics/article


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