Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Soomi Cha"'
Direct measurement of the 26Si(α, p)29P reaction at CRIB for the nucleosynthesis in the X-ray bursts
Autor:
Kodai Okawa, Minju Kim, Kyungyuk Chae, Seiya Hayakawa, Satoshi Adachi, Soomi Cha, Thomas William Chillery, Tatsuya Furuno, Gyungmo Gu, Shutaro Hanai, Nobuaki Imai, David Kahl, Takahiro Kawabata, Chanhee Kim, Dahee Kim, Sohyun Kim, Shigeru Kubono, Minsik Kwag, Jiatai Li, Nanru Ma, Shin’ichiro Michimasa, Uyen Nguyen Kim, Duy Nguyen Ngoc, Kohsuke Sakanashi, Hideki Shimizu, Oana Sirbu, Hidetoshi Yamaguchi, Rin Yokoyama, Qian Zhang
Publikováno v:
EPJ Web of Conferences. 275:02009
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
Autor:
Uwe Greife, Sunghoon Ahn, Michael Scott Smith, K. Y. Chae, Antonios Kontos, Steven D. Pain, Paul J. Thompson, Jolie Cizewski, Ulrike Hager, Jacob Allen, Orlando Gomez, K. L. Jones, D. W. Bardayan, Nata Franco Soares de Bem, A. Lepailleur, Wei Jia Ong, Milan Matos, Rebecca Toomey, Sara Ayoub, Hendrik Schatz, Alison Sachs, Patrick O'Malley, Fernando Montes, Eric Deleeuw, Justin Browne, D. Blankstein, J. C. Blackmon, David Walter, L. E. Linhardt, R. L. Kozub, Zach Meisel, Eunji Lee, Karl Smith, Kelly Chipps, Soomi Cha, Catherine Deibel, Konrad Schmidt, Kyle Schmitt, M. R. Hall
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01043 (2017)
When a neutron star accretes hydrogen and helium from the outer layers of its companion star, thermonuclear burning enables the α p-process as a break out mechanism from the hot CNO cycle. Model calculations predict ( α , p) reaction rates signific