CHEN Xin, SU Jun, ZHANG Hao, CHEN Yinji, SONG Luyang, HU Jun, TIAN Ning, CHEN Size, ZHANG Liyong, HE Jianjun. Energy calibration of low energy proton beam with 18O(p, γ)19F and 27Al(p, γ)28Si resonant reactions[J]. Journal of Beijing Normal University(Natural Science), 2022, 58(5): 733-736. DOI: 10.12202/j.0476-0301.2022163
Citation: CHEN Xin, SU Jun, ZHANG Hao, CHEN Yinji, SONG Luyang, HU Jun, TIAN Ning, CHEN Size, ZHANG Liyong, HE Jianjun. Energy calibration of low energy proton beam with 18O(p, γ)19F and 27Al(p, γ)28Si resonant reactions[J]. Journal of Beijing Normal University(Natural Science), 2022, 58(5): 733-736. DOI: 10.12202/j.0476-0301.2022163

Energy calibration of low energy proton beam with 18O(p, γ)19F and 27Al(p, γ)28Si resonant reactions

  • Low energy, high current proton accelerators, which can run stably for a long period, are crucial for low-energy nuclear astrophysical experiments.The HINEG(high intensity D-T fusion neutron generator) high-voltage platform at Hefei Institute of Physical Sciences, Chinese Academy of Sciences, can provide a proton beam up to 5 mA in the energy range of 70-260 keV.This high current accelerator was used to build a low-energy nuclear astrophysical platform.The beam energy was calibrated with 18O(p, γ)19F and 27Al(p, γ)28Si resonant reactions.Data were analyzed by Geant4 simulation.Simulations showed that for proton beams of 151.3 and 222.8 keV, energy spread was 0.97_-0.05^+0.02 and 1.39_-0.28^+0.12 keV, energy shift was (0.3±0.3) and (1.7±0.1) keV respectively.The HINEG platform satisfies requirements for nuclear astrophysics studies.
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