Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Chillery, Thomas"'
Direct measurement of the 26Si(α, p)29P reaction at CRIB for the nucleosynthesis in the X-ray bursts
Autor:
Okawa Kodai, Kim Minju, Chae Kyungyuk, Hayakawa Seiya, Adachi Satoshi, Cha Soomi, Chillery Thomas William, Furuno Tatsuya, Gu Gyungmo, Hanai Shutaro, Imai Nobuaki, Kahl David, Kawabata Takahiro, Kim Chanhee, Kim Dahee, Kim Sohyun, Kubono Shigeru, Kwag Minsik, Li Jiatai, Ma Nanru, Michimasa Shin’ichiro, Nguyen Kim Uyen, Nguyen Ngoc Duy, Sakanashi Kohsuke, Shimizu Hideki, Sirbu Oana, Yamaguchi Hidetoshi, Yokoyama Rin, Zhang Qian
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02009 (2023)
Several (α, p) reactions with radioactive-ions (RI) in the αp-process are important to characterize X-ray bursts. However, some of them do not have sufficient experimental data, and the 26Si(α, p)29P reaction is one of such reactions. We performed
Externí odkaz:
https://doaj.org/article/121aeffef29b4663a72fa678ceb3210d
Akademický článek
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Autor:
Chillery, Thomas, Hwang, Jongwon, Dozono, Masanori, Imai, Nobuaki, Michimasa, Shin'ichiro, Sumikama, Toshiyuki, Chiga, Nobuyuki, Ota, Shinsuke, Nakayama, Shinsuke, Ahn, Deuk Soon, Beliuskina, Olga, Chikaato, Kazuya, Fukuda, Naoki, Hayakawa, Seiya, Ideguchi, Eiji, Iribe, Kotaro, Iwamoto, Chihiro, Kawase, Shoichiro, Kawata, Keita, Kitamura, Noritaka
Publikováno v:
Progress of Theoretical & Experimental Physics: PTEP; Dec2023, Vol. 2023 Issue 12, p1-11, 11p
Autor:
Chillery Thomas
Publikováno v:
EPJ Web of Conferences, Vol 184, p 02001 (2018)
A discrepancy exists between the 6Li abundances predicted from big bang nucleosynthesis models and those measured in pre-main sequence stars. To further constrain the predicted abundances of 6Li in these stars, high accuracy measurements are required
Externí odkaz:
https://doaj.org/article/c5dfc391f1234492b27f6e84f37bf6e3
Autor:
Okawa, Kodai, Kim, Minju, Chae, Kyungyuk, Hayakawa, Seiya, Adachi, Satoshi, Cha, Soomi, Chillery, Thomas William, Furuno, Tatsuya, Gu, Gyungmo, Hanai, Shutaro, Imai, Nobuaki, Kahl, David, Kawabata, Takahiro, Kim, Chanhee, Kim, Dahee, Kim, Sohyun, Kubono, Shigeru, Kwag, Minsik, Li, Jiatai, Ma, Nanru
Publikováno v:
EPJ Web of Conferences; 2/3/2023, Vol. 275, p1-3, 3p
Autor:
Smith Suzanne V., McCutchan Elizabeth, Gürdal Gülhan, Lister Christopher, Muench Lisa, Nino Michael, Sonzogni Alexandro, Herman Michal, Nobre Gustavo, Cullen Chris, Chillery Thomas, Chowdury Partha, Harding Robert
Publikováno v:
EPJ Web of Conferences, Vol 146, p 09029 (2017)
The accelerator production of platinum isotopes was investigated at the Brookhaven Linac Isotope Producer (BLIP). In this study high purity natural platinum foils were irradiated at 53.2, 65.7, 105.2, 151.9, 162.9 and 173.3.MeV. The irradiated foils
Externí odkaz:
https://doaj.org/article/49f4b44542a542739dce2e4b3ae57519
Underground experimental study finds no evidence of low-energy resonance in the 6Li(p,γ)7Be reaction
Publikováno v:
Chillery, T, Aliotta, M & Bruno, C G & Davinson, T 2020, ' Underground experimental study finds no evidence of low-energy resonance in the 6Li(p,γ)7Be reaction ', Physical Review C, vol. 102, no. 5, 052802(R) . https://doi.org/10.1103/PhysRevC.102.052802
The astrophysical 6Li(p,γ)7Be 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=od______3094::6ef88d482b7c5ac1dbb1c812322f155a
https://www.pure.ed.ac.uk/ws/files/172849401/Piatti_PRC_RC.pdf
https://www.pure.ed.ac.uk/ws/files/172849401/Piatti_PRC_RC.pdf
Autor:
Chillery, Thomas William
Big Bang Nucleosynthesis (BBN) theory coupled with Cosmic Microwave Background measurements provide predictions on the modern day abundances of low mass isotopes, which are then compared to observations from stellar environments. Specifically 6,7Li i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::399e2ba6fdaf174ca221db87fb00c8c3
https://hdl.handle.net/1842/37279
https://hdl.handle.net/1842/37279