Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Stockel, K."'
Autor:
Ciani, G. F., Csedreki, L., Rapagnani, D., Aliotta, M., Balibrea-Correa, J., Barile, F., Bemmerer, D., Best, A., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Chillery, T., Corvisiero, P., Cristallo, S., Davinson, T., Depalo, R., DiLeva, A., Elekes, Z., Ferraro, F., Fiore, E., Formicola, A., Fulop, Zs., Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy., Imbriani, G., Junker, M., Lugaro, M., Marigo, P., Masha, E., Menegazzo, R., Mossa, V., Pantaleo, F. R., Paticchio, V., Perrino, R., Piatti, D., Prati, P., Schiavulli, L., Stockel, K., Straniero, O., Szucs, T., Takacs, M. P., Terrasi, F., Vescovi, D., Zavatarelli, S .
One of the main neutron sources for the astrophysical s-process is the reaction 13C({\alpha},n)16O, taking place in thermally pulsing Asymptotic Giant Branch stars at temperatures around 90 MK. To model the nucleosynthesis during this process the rea
Externí odkaz:
http://arxiv.org/abs/2110.00303
Autor:
Ciani, G. F., Csedreki, L., Balibrea-Correa, J., Best, A., Aliotta, M., Barile, F., Bemmerer, D., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Chillery, T., Colombetti, P., Corvisiero, P., Davinson, T., Depalo, R., Di Leva, A., Di Paolo, L., Elekes, Z., Ferraro, F., Fiore, E. M., Formicola, A., Fulop, Zs., Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy., Imbriani, G., Junker, M., Kochanek, I., Lugaro, M., Marigo, P., Masha, E., Menegazzo, R., Mossa, V., Pantaleo, F. R., Paticchio, V., Perrino, R., Piatti, D., Prati, P., Schiavulli, L., Stockel, K., Straniero, O., Szucs, T., Takacs, M. P., Terrasi, F., Trezzi, D., Zavatarelli, S.
Publikováno v:
The European Physical Journal A volume 56, Article number: 75 (2020)
Direct measurements of reaction cross-sections at astrophysical energies often require the use of solid targets able to withstand high ion beam currents for extended periods of time. Thus, monitoring target thickness, isotopic composition, and target
Externí odkaz:
http://arxiv.org/abs/2001.08744
Akademický článek
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Autor:
Csedreki L., Ciani G. F., Balibrea-Correa J., Best A., Aliotta M., Barile F., Bemmerer D., Boeltzig A., Broggini C., Bruno C. G., Caciolli A., Cavanna F., Chillery T., Colombetti P., Corvisiero P., Davinson T., Depalo R., Di Leva A., Elekes Z., Ferraro F., Fiore E. M., Formicola A., Fulop Z., Gervino G., Guglielmetti A., Gustavino C., Gyurky G., Imbriani G., Janas Z., Junker M., Kochanek I., Lugaro M., Marigo P., Masha E., Mazzocchi C., Menegazzo R., Mossa V., Pantaleo F. R., Paticchio V., Perrino R., Piatti D., Prati P., Schiavulli L., Stockel K., Straniero O., Szucs T., Takacs M. P., Terrasi F., Zavatarelli S.
Publikováno v:
Csedreki, L, Ciani, G F, Balibrea-Correa, J, Best, A, Aliotta, M, Barile, F, Bemmerer, D, Boeltzig, A, Broggini, C, Bruno, C G, Caciolli, A, Cavanna, F, Chillery, T, Colombetti, P, Corvisiero, P, Davinson, T, Depalo, R, Di Leva, A, Elekes, Z, Ferraro, F, Fiore, E M, Formicola, A, Fulop, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyurky, G, Imbriani, G, Janas, Z, Junker, M, Kochanek, I, Lugaro, M, Marigo, P, Masha, E, Mazzocchi, C, Menegazzo, R, Mossa, V, Pantaleo, F R, Paticchio, V, Perrino, R, Piatti, D, Prati, P, Schiavulli, L, Stockel, K, Straniero, O, Szucs, T, Takacs, M P, Terrasi, F & Zavatarelli, S 2021, ' Characterization of the LUNA neutron detector array for the measurement of the 13C(α,n)16O reaction ', Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 994, 165081 . https://doi.org/10.1016/j.nima.2021.165081
We introduce the LUNA neutron detector array developed for the investigation of the 13C(α, n)16O reaction towards its astrophysical s-process Gamow peak in the low-background environment of the Laboratori Nazionali del Gran Sasso (LNGS). Eighteen 3H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::be23f4e14614e8637eb11af34cb0b8a2
https://hdl.handle.net/20.500.11820/178ba5e8-32e7-42c1-b261-7e49db21e167
https://hdl.handle.net/20.500.11820/178ba5e8-32e7-42c1-b261-7e49db21e167
Autor:
Ciani, G. F., Csedreki, L., Rapagnani, D., Aliotta, M., Balibrea-Correa, J., Barile, F., Bemmerer, D., Best, A., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Chillery, T., Colombetti, P., Corvisiero, P., Cristallo, S., Davinson, T., Depalo, R., Di Leva, A., Elekes, Z., Ferraro, F., Fiore, E., Formicola, A., Fulop, Zs., Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, G., Imbriani, G., Junker, M., Lugaro, M., Marigo, P., Masha, E., Menegazzo, R., Mossa, V., Pantaleo, F. R., Paticchio, V., Perrino, R., Piatti, D., Prati, P., Schiavulli, L., Stockel, K., Straniero, O., Szucs, T., Takacs, M. P., Terrasi, F., Vescovi, D., Zavatarelli, S.
Publikováno v:
arXiv:2110.00303v1 [nucl-ex]: https://arxiv.org/pdf/2110.00303.pdf
Physical Review Letters 127(2021), 152701
Physical Review Letters 127(2021), 152701
One of the main neutron sources for the astrophysical s process is the reaction ^{13}C(α,n)^{16}O, taking place in thermally pulsing asymptotic giant branch stars at temperatures around 90 MK. To model the nucleosynthesis during this process the rea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid_dedup__::f3eea28dc9acd2304e2e4d9709d867fd
http://hdl.handle.net/11588/876370
http://hdl.handle.net/11588/876370
Autor:
Piatti, D., Chillery, T., Depalo, R., Aliotta, M., Bemmerer, D., Best, A., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Ciani, G. F., Corvisiero, P., Csedreki, L., Davinson, T., Di Leva, A., Elekes, Z., Ferraro, F., Fiore, E. M., Formicola, A., Fulop, Zs., Gervino, G., Gnech, A., Guglielmetti, A., Gustavino, C., Gyurky, Gy., Imbriani, G., Junker, M., Kochanek, I., Lugaro, M., Marcucci, L. E., Marigo, P., Masha, E., Menegazzo, R., Mossa, V., Pantaleo, F. R., Paticchio, V., Perrino, R., Prati, P., Schiavulli, L., Stockel, K., Straniero, O., Szucs, T., Takacs, M. P., Zavatarelli, S.
The astrophysical Li6(p,γ)Be7 reaction occurs during Big Bang nucleosynthesis and the pre-main sequence and main sequence phases of stellar evolution. The low-energy trend of its cross section remains uncertain, since different measurements have pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::69b3ec96b948dca982da11baed29e418
http://hdl.handle.net/11588/827427
http://hdl.handle.net/11588/827427
Autor:
Ciani, G. F., Csedreki, L., Balibrea-Correa, J., Best, A., Aliotta, M., Barile, F., Bemmerer, D., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Cavanna, F., Chillery, T., Colombetti, P., Corvisiero, P., Davinson, T., Depalo, R., Di Leva, A., Di Paolo, L., Elekes, Z., Ferraro, F., Fiore, E. M., Formicola, A., Fulop, Z., Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, G., Imbriani, G., Junker, M., Kochanek, I., Lugaro, M., Marigo, P., Masha, E., Menegazzo, R., Mossa, V., Pantaleo, F. R., Paticchio, V., Perrino, R., Piatti, D., Prati, P., Schiavulli, L., Stockel, K., Straniero, O., Szucs, T., Takacs, M. P., Terrasi, F., Trezzi, D., Zavatarelli, S.
Publikováno v:
European Physical Journal A 56(2021), 75
Ciani, G F, Csedreki, L, Balibrea-Correa, J, Best, A, Aliotta, M, Barile, F, Bemmerer, D, Boeltzig, A, Broggini, C, Bruno, C G, Caciolli, A, Cavanna, F, Chillery, T, Colombetti, P, Corvisiero, P, Davinson, T, Depalo, R, Di Leva, A, Di Paolo, L, Elekes, Z, Ferraro, F, Fiore, E M, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyurky, G, Imbriani, G, Junker, M, Kochanek, I, Lugaro, M, Marigo, P, Masha, E, Menegazzo, R, Mossa, V, Pantaleo, F R, Paticchio, V, Perrino, R, Piatti, D, Prati, P, Schiavulli, L, Stöckel, K, Straniero, O, Szucs, T, Takács, M P, Terrasi, F, Trezzi, D & Zavatarelli, S 2020, ' A new approach to monitor 13C-targets degradation in situfor 13C(α,n)16O cross-section measurements at LUNA ', European Physical Journal A: Hadrons and Nuclei . https://doi.org/10.1140/epja/s10050-020-00077-0
Ciani, G F, Csedreki, L, Balibrea-Correa, J, Best, A, Aliotta, M, Barile, F, Bemmerer, D, Boeltzig, A, Broggini, C, Bruno, C G, Caciolli, A, Cavanna, F, Chillery, T, Colombetti, P, Corvisiero, P, Davinson, T, Depalo, R, Di Leva, A, Di Paolo, L, Elekes, Z, Ferraro, F, Fiore, E M, Formicola, A, Fülöp, Z, Gervino, G, Guglielmetti, A, Gustavino, C, Gyurky, G, Imbriani, G, Junker, M, Kochanek, I, Lugaro, M, Marigo, P, Masha, E, Menegazzo, R, Mossa, V, Pantaleo, F R, Paticchio, V, Perrino, R, Piatti, D, Prati, P, Schiavulli, L, Stöckel, K, Straniero, O, Szucs, T, Takács, M P, Terrasi, F, Trezzi, D & Zavatarelli, S 2020, ' A new approach to monitor 13C-targets degradation in situfor 13C(α,n)16O cross-section measurements at LUNA ', European Physical Journal A: Hadrons and Nuclei . https://doi.org/10.1140/epja/s10050-020-00077-0
Direct measurements of reaction cross-sections at astrophysical energies often require the use of solid targets able to withstand high ion beam currents for extended periods of time. Thus, monitoring target thickness, isotopic composition, and target
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::516585ae24e47913272f12a917781e71
http://hdl.handle.net/2318/1785053
http://hdl.handle.net/2318/1785053
Akademický článek
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Akademický článek
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