Photoneutron Reactions in Nuclear Astrophysics

NUBA Conference Series -1: Nuclear Physics and Astrophysics

物理学;天文学

Utsunomiya, H.^1,2 ; Goriely, S.^1,2,3 ; Filipescu, D.M.^1 ; Tesileanu, O.^4 ; Gheorghe, I.^1 ; Glodariu, T.^5 ; Nyhus, H.-T.^1 ; Renstrøm, T.^6 ; Lui, Y.-W.^7 ; Shima, T.^8 ; Takahisa, K.^8 ; Miyamoto, S.^9

Department of Physics, Konan University, Kobe, Japan^1

Center of Nuclear Science, University of Tokyo, Saitama, Japan^2

Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Brussels, Belgium^3

Extreme Light Infrastructure Nuclear Physics, Bucharest-Magurele, Romania^4

National Institute for Physics and Nuclear Engineering Horia Hulubei, Bucharest- Magurele, Romania^5

Department of Physics, University of Oslo, Oslo, Norway^6

Texas AandM University, College Station

TX, United States^7

Research Center for Nuclear Physics, Osaka University, Osaka, Japan^8

Laboratory of Advanced Science and Technology for Industry, University of Hyogo, Hyogo, Japan^9

关键词: Inverse Compton scattering;    Laser photons;    Nuclear astro-physics;    Relativistic electron;    S-process;    Synchrotron radiation facility;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/590/1/012023/pdf
DOI  :  10.1088/1742-6596/590/1/012023

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

Highly-monochromatic γ-ray beams are produced at the NewSUBARU synchrotron radiation facility by the inverse Compton scattering of laser photons from relativistic electrons. The latest s-process study in nuclear astrophysics with the γ-ray beam is presented.