Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Gy��rky, Gy."'
The prediction of stellar ($��$,$��$) reaction rates for heavy nuclei is based on the calculation of ($��$,$��$) cross sections at sub-Coulomb energies. These rates are essential for modeling the nucleosynthesis of so-called $p$-nucle
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d9f25d51df7ec4247463d19eece9cf5
The precise knowledge of the half-life of the reaction product is of crucial importance for a nuclear reaction cross section measurement carried out with the activation technique. The cross section of the $^{92}$Mo($��$,n)$^{95}$Ru reaction was m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6166375f5472b74251117fa6212ad00
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:
https://explore.openaire.eu/search/publication?articleId=doi_________::01bb6505116ca2101ef4bf0ba2b13209
Autor:
Gy��rky, Gy., Hal��sz, Z., Kiss, G. G., Sz��cs, T., Cs��k, A., T��r��k, Zs., Husz��nk, R., Kohan, M. G., Wagner, L., F��l��p, 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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::603ce8eb71d91b8394956af40799dbe2
http://arxiv.org/abs/1907.07446
http://arxiv.org/abs/1907.07446
The $^3$He($��$,$��$)$^7$Be reaction is a widely studied nuclear reaction; however, it is still not understood with the required precision. It has a great importance both in Big Bang nucleosynthesis and in solar hydrogen burning. The low mass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12222dec4374b4992cbdf2e02b6c2eb3
Autor:
Sz��cs, T., Mohr, P., Gy��rky, Gy., Hal��sz, Z., Husz��nk, R., Kiss, G. G., Szegedi, T. N., T��r��k, Zs., F��l��p, Zs.
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:
https://explore.openaire.eu/search/publication?articleId=doi_________::2f8f84475ef0f801b493b66737585c7c
Autor:
Szegedi, T. N., Kiss, G. G., ��ks��z, I., Sz��cs, T., Gy��rky, Gy., Elekes, Z., Somorjai, E., F��l��p, Zs.
In order to provide data for the simulation of the astrophysical $��$-process, the cross section measurement of the $^{124}$Xe(p,$��$)$^{125}$Cs reaction is in progress at MTA Atomki using the activation technique. Precise information on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::38a4082c9f5ba38b2f51c5d4bc33b502
Autor:
Bemmerer, D., Cavanna, F., Depalo, R., Aliotta, M., Anders, M., Boeltzig, A., Broggini, C., Bruno, C., Caciolli, A., Corvisiero, P., Davinson, T., Elekes, Z., Ferraro, F., Formicola, A., F��l��p, Zs., Gervino, G., Guglielmetti, A., Gustavino, C., Gy��rky, Gy., Menegazzo, R., Mossa, V., Pantaleo, F. R., Prati, P., Scott, D. A., Straniero, O., Sz��cs, T., Tak��cs, M. P., Trezzi, D.
When deriving resonance strengths using the thick-target yield approximation, for very narrow resonances it may be necessary to take beam energy straggling into account. This applies to gas targets of a few keV width, especially if there is some addi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e724e65e801e22acda528150248437f3
Autor:
Korkulu, Z., ��zkan, N., Kiss, G. G., Sz��cs, T., Gy��rky, Gy., F��l��p, Zs., G��ray, R. T., Hal��sz, Z., Rauscher, T., Somorjai, E., T��r��k, Zs., Yal����n, C.
The aim of the present work is to measure the $^{121}$Sb($��,��$)$^{125}$I, $^{121}$Sb($��$,n)$^{124}$I, and $^{123}$Sb($��$,n)$^{126}$I reaction cross sections. The $��$-induced reactions on natural and enriched antimony targets
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8798d06a17bba7bc5cdf54f9d2b34190
Autor:
Ferraro, F., Tak��cs, M. P., Piatti, D., Mossa, V., Aliotta, M., Bemmerer, D., Best, A., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Chillery, T., Ciani, G. F., Corvisiero, P., Csedreki, L., Davinson, T., Depalo, R., D'Erasmo, G., Di Leva, A., Elekes, Z., Fiore, E. M., Formicola, A., F��l��p, Zs., Gervino, G., Guglielmetti, A., Gustavino, C., Gy��rky, Gy., Imbriani, G., Junker, M., Kochanek, I., Lugaro, M., Marcucci, L. E., Marigo, P., Menegazzo, R., Pantaleo, F. R., Paticchio, V., Perrino, R., Prati, P., Schiavulli, L., St��ckel, K., Straniero, O., Sz��cs, T., Trezzi, D., Zavatarelli, S.
The experimental study of nuclear reactions of astrophysical interest is greatly facilitated by a low-background, high-luminosity setup. The Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator offers ultra-low cosmic-ray induced
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cd3d62a51d0f7e3ce530312e3ae31c79