1 research outputs found
Simulation of Star configurations in the BINA detector
Star Anomaly is one of the most intriguing and unsolved discrepancies
between theoretical calculations and experimental data observed in the domain
of few-nucleon systems at low energies. Previous and upcoming measurements
of the breakup reaction with the use of the BINA detector enable
systematic studies of the Star configurations at intermediate energies. A
dedicated simulation was developed to study feasibility of registering such
events with the required accuracy and to support the future data analysis.
An additional rotation angle has been introduced to parametrise the Star
configurations. First results concerning the acceptance of certain segments
of BINA for registering the Star configurations are presented