Description of three-body scattering for astrophysics

Details Description of three-body scattering for astrophysics Description of three-body scattering for astrophysics

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..445k&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Statistics

Applications

Scattering Of Acoustic Waves, Cosmic Ray Nucleosynthesis, Chemical Kinetics And Reactions: Special Regimes And Techniques

Scientific paper

A new and simple discription of the three-body scattering states, which is based on the Lippmann-Schwinger equation and the complex scaling method, is developed. As applications of this method, the energy distribution of the E1 transition strength for 6He is calculated. It is also shown that the correlations of subsystems in 6He are well reproduced.

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