skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Development of a new bremsstrahlung source for nuclear astrophysics

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3485177· OSTI ID:21426535
 [1];  [2];  [3];  [4]
  1. Meme Media Laboratory, Hokkaido University 060-8628 Sapporo (Japan)
  2. Department of Physics, Faculty of Science, Hokkaido University 060-0810 Sapporo (Japan)
  3. Division of Quantum Science and Engineering, Graduate School of Engineering, Hokkaido University 060-8628 Sapporo (Japan)
  4. Department of Computer Science, Kitami Institute of Technology 090-8507 Kitami (Japan)

Nuclear reaction rate for photodisintegration and their inverse, charged particle and neutron capture reactions, are important input quantities for stellar nucleosynthesis. In order to evaluate reaction rates precisely, both nuclear experiment and model prediction are needed. Recently, real photon-beam is used as powerful tools for astrophysics. In this work, current status of the development of a new bremsstrahlung {gamma}-ray source with the electron linear accelerator at Hokkaido University will be presented.

OSTI ID:
21426535
Journal Information:
AIP Conference Proceedings, Vol. 1269, Issue 1; Conference: OMEG-2010: 10. international symposium on origin of matter and evolution of galaxies, Osaka (Japan), 8-10 Mar 2010; Other Information: DOI: 10.1063/1.3485177; (c) 2010 American Institute of Physics; ISSN 0094-243X
Country of Publication:
United States
Language:
English