Pregled bibliografske jedinice broj: 1183069
First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process
First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process // EPJ Web of Conferences 260 / Liu, W. ; Wang, Y. ; Guo, B. ; Tang, X. ; Zeng, S. (ur.).
Chengdu, Kina, 2022. 11026, 8 doi:10.1051/epjconf/202226011026 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
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Naslov
First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process
Autori
Babiano-Suarez, V. ; ... ; Bosnar, Damir ; ... ; Žugec, Petar
Kolaboracija
N_TOF Collaboration
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
EPJ Web of Conferences 260
/ Liu, W. ; Wang, Y. ; Guo, B. ; Tang, X. ; Zeng, S. - , 2022
Skup
The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
Mjesto i datum
Chengdu, Kina, 21.09.2021. - 25.09.2021
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
80Se, neutron capture, n_TOF, s-process
Sažetak
Most elements heavier than iron have been generated in the stellar media by means of neutron capture reactions, approximately half are produced by the slow neutron capture or s-process. Radiative neutron capture cross section measurements are of fundamental importance for the study of this mechanism. In this contribution we present a brief summary on the measurement and results for the 80Se(n, γ) cross-section. The experiment was carried out at CERN n_TOF EAR1 via the time of flight (ToF) technique, using four C6D6 scintillation detectors with very fast response. More than a hundred new resonances have been analyzed for the first time with a high accuracy. The MACS obtained at kT = 8 keV is 36% smaller than the recommended value in KADoNiS. Some of the astrophysical implications of this result are elucidated in this contribution.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb