Abstract
Within the framework of the modified potential cluster model with forbidden states, radiative 3He3H capture at low and astrophysical energies is considered. It is shown that on the basis of potentials which are matched with scattering phase shifts and the energy of the bound state, overall success is obtained in reproducing the available experimental data. On the basis of the obtained total cross sections, a calculation of the astrophysical S-factor and the capture reaction rate has been performed. All of the obtained results are approximated by curves of a definite type, which simplifies their use in applied studies.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
