Zobrazeno 1 - 10
of 104
pro vyhledávání: '"Huszank, R."'
Autor:
Gyürky, Gy., Halász, Z., Kiss, G. G., Szücs, T., Huszánk, R., Török, Zs., Fülöp, Zs., Rauscher, T., Travaglio, C.
Publikováno v:
Journal of Physics G: Nuclear and Particle Physics 48 (2021) 105202
The synthesis of heavy, proton rich isotopes is a poorly understood astrophysical process. Thermonuclear (type Ia) supernova explosions are among the suggested sites and the abundance of some isotopes present in the early solar system may be used to
Externí odkaz:
http://arxiv.org/abs/2108.10006
Lighter heavy elements beyond iron and up to around silver can form in neutrino-driven ejecta in core-collapse supernovae and neutron star mergers. Slightly neutron-rich conditions favour a weak r-process that follows a path close to stability. There
Externí odkaz:
http://arxiv.org/abs/2009.13169
Autor:
Szücs, T., Mohr, P., Gyürky, Gy., Halász, Z., Huszánk, R., Kiss, G. G., Szegedi, T. N., Török, Zs., Fülöp, Zs.
Publikováno v:
Phys. Rev. C 100, 065803 (2019)
Statistical model calculations have to be used for the determination of reaction rates in large-scale reaction networks for heavy-element nucleosynthesis. A basic ingredient of such a calculation is the a-nucleus optical model potential. Several diff
Externí odkaz:
http://arxiv.org/abs/1910.09888
Autor:
Gyürky, Gy., Halász, Z., Kiss, G. G., Szücs, T., Csík, A., Török, Zs., Huszánk, R., Kohan, M. G., Wagner, L., Fülöp, Zs.
The 14N(p,gamma)15O reaction plays a vital role in various astrophysical scenarios. Its reaction rate must be accurately known in the present era of high precision astrophysics. The cross section of the reaction is often measured relative to a low en
Externí odkaz:
http://arxiv.org/abs/1907.07446
Publikováno v:
Phys. Rev. C 97, 055803 (2018)
[Background] Alpha-nucleus optical potentials are basic ingredients of statistical model calculations used in nucleosynthesis simulations. While the nucleon+nucleus optical potential is fairly well known, for the alpha+nucleus optical potential sever
Externí odkaz:
http://arxiv.org/abs/1805.07533
Autor:
Gyürky, Gy., Ornelas, A., Fülöp, Zs., Halász, Z., Kiss, G. G., Szücs, T., Huszánk, R., Hornyák, I., Rajta, I., Vajda, I.
Publikováno v:
Phys. Rev. C 95, 035805 (2017)
The 17O(p,g)18F reaction plays an important role in hydrogen burning processes in different stages of stellar evolution. The rate of this reaction must therefore be known with high accuracy in order to provide the necessary input for astrophysical mo
Externí odkaz:
http://arxiv.org/abs/1703.03184
Publikováno v:
In Radiation Physics and Chemistry March 2021 180
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 1 July 2019 450:364-368
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 15 March 2019 443:48-56
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 1 November 2015 362:167-171