Abstract
AbstractAnalysis of the data acquired with the BINA detector system in $$^1$$
1
H(d, pp)n reaction at the beam energy of 80 MeV/nucleon makes a systematic analysis of the star configurations possible. This paper shows the preliminary cross section of the Forward-Plane Star (FPS) configuration with the neighbouring configurations.
Publisher
Springer Science and Business Media LLC
Subject
Atomic and Molecular Physics, and Optics