The Feasibility of Studying 44Ti(α, p)47V Reaction at Astrophysical Energies
The Feasibility of Studying 44Ti(α, p)47V Reaction at Astrophysical Energies
Al-Abdullah, T.; Bemmerer, D.; Elekes, Z.; Schumann, D.
Abstract
The gamma-ray lines from the decay of 44Ti have been observed by space-based gamma-ray telescopes from two supernova remnants. It is believed that the 44Ti(α, p)47V reaction dominates the destruction of 44Ti. This work presents a possible technique to determine its reaction rate in forward kinematics at astrophysically relevant energies. Several online and offline measurements in parallel with Monte Carlo simulations were performed to illustrate the feasibility of performing this reaction. The results will be discussed.
Beteiligte Forschungsanlagen
- Ionenstrahlzentrum DOI: 10.17815/jlsrf-3-159
Verknüpfte Publikationen
- DOI: 10.17815/jlsrf-3-159 is cited by this (Id 27528) publication
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Journal of Physics: Conference Series 940(2018), 012028
DOI: 10.1088/1742-6596/940/1/012028
Permalink: https://www.hzdr.de/publications/Publ-27528