Now showing items 1-4 of 4

    • Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies 

      Yalçin, C.; Özkan, N.; Güray, R. T.; Gyürky, Gy; Kiss, G. G.; Szücs, T.; Haiász, Z.; Fülöp, Zs; Farkas, J.; Somorjai, E.; Korkulu, Z.; Rauscher, T. (2016-01-05)
      Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. ...
    • Investigation of alpha-induced reactions on I-127 for the astrophysical gamma process 

      Kiss, G. G.; Szuecs, T.; Toeroek, Zs.; Korkulu, Z.; Gyuerky, Gy.; Halasz, Z.; Fueloep, Zs.; Somorjai, E.; Rauscher, T. (2012-09-04)
      Background: The. process in core-collapse supernova explosions is thought to explain the origin of proton-rich isotopes between Se and Hg, the so-called p nuclei. The majority of the reaction rates for gamma process reaction ...
    • Investigation of α -induced reactions on Sb isotopes relevant to the astrophysical γ process 

      Korkulu, Z.; Özkan, N.; Kiss, G. G.; Szücs, T.; Gyürky, Gy; Fülöp, Zs; Güray, R. T.; Halász, Z.; Rauscher, T.; Somorjai, E.; Török, Zs; Yalçln, C. (2018-04-16)
      Background: The reaction rates used in γ-process nucleosynthesis network calculations are mostly derived from theoretical, statistical model cross sections. Experimental data is scarce for charged particle reactions at ...
    • Test of statistical model cross section calculations for α -induced reactions on Ag 107 at energies of astrophysical interest 

      YalçIn, C.; Gyürky, Gy; Rauscher, T.; Kiss, G. G.; Özkan, N.; Güray, R. T.; Halász, Z.; Szücs, T.; Fülöp, Zs; Farkas, J.; Korkulu, Z.; Somorjai, E. (2015-03-16)
      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 ...