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.
|Journal||Journal of Physics: Conference Series|
|Publication status||Published - Jan 31 2018|
|Event||7th Nuclear Physics in Astrophysics Conference, NPA 2015 - York, United Kingdom|
Duration: May 18 2015 → May 22 2015
ASJC Scopus subject areas
- Physics and Astronomy(all)