Development of a new bremsstrahlung source for nuclear astrophysics

Details Development of a new bremsstrahlung source for nuclear astrophysics Development of a new bremsstrahlung source for nuclear astrophysics

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..394m&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Physics

Nuclear Physics

Nuclear Experiment

Nucleosynthesis, White Dwarfs, Supernovae, Compton Effect, Monte Carlo Methods, Cosmic Ray Nucleosynthesis, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Supernovae, Neutron Inelastic Scattering, Monte Carlo Models

Scientific paper

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 γ-ray source with the electron linear accelerator at Hokkaido University will be presented.

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