Zobrazeno 1 - 10
of 331
pro vyhledávání: '"Xu S.W."'
Autor:
Yamaguchi H., Hayakawa S., Ma N.R., Shimizu H., Okawa K., Zhang Q., Yang L., Kahl D., La Cognata M., Lamia L., Abe K., Beliuskina O., Cha S.M., Chae K.Y., Cherubini S., Figuera P., Ge Z., Gulino M., Hu J., Inoue A., Iwasa N., Kim A., Kim D., Kiss G., Kubono S., La Commara M., Lattuada M., Lee E.J., Moon J.Y., Palmerini S., Parascandolo C., Park S.Y., Phong V.H., Pierroutsakou D., Pizzone R.G., Rapisarda G.G., Romano S., Spitaleri C., Tang X.D., Trippella O., Tumino A., Zhang N.T., Lam Y.H., Heger A., Jacobs A.M., Xu S.W., Ma S.B., Ru L.H., Liu E.Q., Liu T., Hamill C.B., Murphy A. St J., Su J., Fang X., Kwag M.S., Duy N.N., Uyen N.K., Kim D.H., Liang J., Psaltis A., Sferrazza M., Johnston Z., Li Y.Y.
Publikováno v:
EPJ Web of Conferences, Vol 275, p 01015 (2023)
Astrophysical reactions involving radioactive isotopes (RI) often play an important role in high-temperature stellar environments. The experimental studies on the reaction rates for those are still limited mainly due to the technical difficulties in
Externí odkaz:
https://doaj.org/article/bddb2deee4b24a159b646a7fe3f55ce2
First measurement of 25Al+p resonant scattering relevant to the astrophysical reaction 22Mg(α,p)25Al
Autor:
Hu J., Yamaguchi H., Lam Y.H., Heger A., Kahl D., Jacobs A.M., Johnston Z., Xu S.W., Zhang N.T., Ma S.B., Ru L.H., Liu E.Q., Liu T., Hayakawa S., Yang L., Shimizu H., Hamill C.B., Murphy A. StJ., Su J., Fang X., Chae K.Y., Kwag M.S., Cha S.M., Duy N.N., Uyen N.K., Kim D.H., Pizzone R.G., La Cognata M., Cherubini S., Romano S., Tumino A., Liang J., Psaltis A., Sferrazza M., Kim D., Li Y.Y., Kubono S.
Publikováno v:
EPJ Web of Conferences, Vol 260, p 05001 (2022)
Type I X-ray bursts (XRBs) are the most frequently observed thermonuclear explosions in nature. The 22Mg(α,p)25Al reaction plays a critical role in XRB models. However, experimental information is insufficient to deduce a precise 22Mg(α,p)25Al reac
Externí odkaz:
https://doaj.org/article/47a812a3f0394ca8996e436339d2f1bd
Autor:
Zhang L.Y., Su J., He J.J., Wiescher M., deBoer R.J., Kahl D., Chen Y.J., Li X.Y., Wang J.G., Zhang L., Cao F.Q., Zhang H., Zhang Z.C., Jiao T.Y., Sheng Y.D., Wang L.H., Song L.Y., Jiang X.Z., Li Z.M., Li E.T., Wang S., Lian G., Li Z.H., Tang X.D., Zhao H.W., Sun L.T., Wu Q., Li J.Q., Cui B.Q., Chen L.H., Ma R.G., Guo B., Xu S.W., Li J.Y., Qi N.C., Sun W.L., Guo X.Y., Zhang P., Chen Y.H., Zhou Y., Zhou J.F., He J.R., Shang C.S., Li M.C., Zhou X.H., Zhang Y.H., Zhang F.S., Hu Z.G., Xu H.S., Cheng J.P., Liu W.P.
Publikováno v:
EPJ Web of Conferences, Vol 260, p 08004 (2022)
The 19F(p, αγ)16O reaction is of crucial importance for Galactic 19F abundances and CNO cycle loss in first generation Population III stars. Due to its extremely small cross sections, the 19F(p, αγ)16O reaction has not been measured in the low en
Externí odkaz:
https://doaj.org/article/7fa688e3b0c540faa48695b24f23a2cc
Autor:
Yamaguchi H., Hayakawa S., Ma N.R., Shimizu H., Okawa K., Yang L., Kahl D., La Cognata M., Lamia L., Abe K., Beliuskina O., Cha S.M., Chae K.Y., Cherubini S., Figuera P., Ge Z., Gulino M., Hu J., Inoue A., Iwasa N., Kim A., Kim D., Kiss G., Kubono S., La Commara M., Lattuada M., Lee E.J., Moon J.Y., Palmerini S., Parascandolo C., Park S.Y., Phong V. H., Pierroutsakou D., Pizzone R.G., Rapisarda G.G., Romano S., Spitaleri C., Tang X.D., Trippella O., Tumino A., Zhang N.T., Lam Y.H., Heger A., Jacobs A.M., Xu S.W., Ma S.B., Ru L.H., Liu E.Q., Liu T., Hamill C.B., St J. Murphy A., Su J., Fang X., Kwag M.S., Duy N.N., Uyen N.K., Kim D.H., Liang J, Psaltis A., Sferrazza M., Johnston Z., Li Y.Y.
Publikováno v:
EPJ Web of Conferences, Vol 260, p 03003 (2022)
Experimental studies on astrophysical reactions involving radioactive isotopes (RI) often accompany technical challenges. Studies on such nuclear reactions have been conducted at the low-energy RI beam separator CRIB, operated by Center for Nuclear S
Externí odkaz:
https://doaj.org/article/b0873e80403540bca7a4d103f879a4d0
Autor:
Xu, J.M., Ding, M.M., Yu, T., Shi, S.H., Xu, S.W., Guan, Y.F., Peng, X.W., Zhang, B.X., Zuo, J.C.
Publikováno v:
In Advances in Space Research 1 September 2024 74(5):2092-2116
Autor:
Wang Y.B., Jin S.J., Jing L., Han Z.Y., Bai X.X., Guo B., Li Y.J., Li Z.H., Lian G., Su J., Sun L.J., Yan S.Q., Zeng S., Liu W.P., Yamaguchi H., Kubono S., Hu J., Kahl D., He J.J, Wang J.S., Tang X.D., Xu S.W., Ma P., Zhang N.T., Bai Z., Huang M.R., Jia B.L., Jin S.L., Ma J.B., Ma S.B., Ma W.H., Yang Y.Y., Zhang L.Y., Jung H.S., Moon J.Y., Lee C.S., Teranishi T., Wang H.W., Ishiyama H., Iwasa N., Komatsubara T., Brown B.A.
Publikováno v:
EPJ Web of Conferences, Vol 109, p 04010 (2016)
22Na is an important isotope for the study of extinct radioactivity, meanwhile its sufficiently long half life provides the possibility to observe live 22Na in nearby nova explosions. The 22Na(p,γ) 23Mg is one of the key reactions that influence the
Externí odkaz:
https://doaj.org/article/a50d98818a394b4182d8e700dc57108a
Publikováno v:
In Advances in Space Research 1 July 2022 70(1):70-84
Publikováno v:
In Marine Structures July 2021 78
Publikováno v:
In Journal of Alloys and Compounds 25 October 2019 806:71-78
Publikováno v:
In Acta Materialia November 2018 160:97-108