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Photoneutron Reactions in Nuclear Astrophysics

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, , Citation H Utsunomiya et al 2015 J. Phys.: Conf. Ser. 590 012023 DOI 10.1088/1742-6596/590/1/012023

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hiro@konan-u.ac.jp

Author affiliations

1 Department of Physics, Konan University, Kobe, Japan

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

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

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

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

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

7 Texas A&M University, College Station, Texas, USA

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

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

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1742-6596/590/1/012023

Abstract

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.

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10.1088/1742-6596/590/1/012023