Abstract

In this report, overview of the new installed Pelletron 5SDH-2 accelerator at Hanoi University of Science, Vietnam and possibilities for performing astrophysics-related nuclear reactions based on this accelerator will be described. In addition to that, some preliminary simulation results for designing and optimizing the experimental set-up in studying reactions 10B(α, p)13C with projectile energies in the Gamow-window will be shown.

Highlights

  • Pelletron 5SHD-2 acclerator installed 2011 at Hanoi Unversity of Science (HUS) is 1.7 MV tandem electronstatic type, manufactured by National Electrostatic Corporation, USA

  • Other analysis technique is Rutherford backscattering (RBS) using low energy α, which is useful to determine the composition of a thin layer surface

  • The seconde module, which inherits from G4HadronicInteraction base clase, generates the kinematics distribution for final state particles

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Summary

Introduction

Pelletron 5SHD-2 acclerator installed 2011 at Hanoi Unversity of Science (HUS) is 1.7 MV tandem electronstatic type, manufactured by National Electrostatic Corporation, USA. Recently a program to study astrophysics-related nuclear reaction induced by low energy proton and α beam within Gamow window has been launched. Some reactions such 7Be(α, γ)11C and 10B(α, p)13C... These models fails to generate acceptable result for energy spectrum of proton from 10B(α, p)13C reaction (see Fig.). The first is dedicated to calculate the interaction cross-section and the second calculates the final state particle as well as their kinematic distribution. The seconde module, which inherits from G4HadronicInteraction base clase, generates the kinematics distribution for final state particles.

Simulation results and discussion
Findings
Conclusion
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