The Feasibility of Studying 44Ti(α, p)47V Reaction at Astrophysical Energies

Tariq Al-Abdullah; D. Bemmerer; Z. Elekes; D. Schumann

doi:10.1088/1742-6596/940/1/012028

The Feasibility of Studying ⁴⁴Ti(α, p)⁴⁷V Reaction at Astrophysical Energies

Tariq Al-Abdullah
, D. Bemmerer
, Z. Elekes
, D. Schumann

Research output: Contribution to journal › Conference article › peer-review

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.

Original language	English
Article number	012028
Journal	Journal of Physics: Conference Series
Volume	940
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/940/1/012028
State	Published - 31 Jan 2018
Externally published	Yes

Bibliographical note

Publisher Copyright:
© Published under licence by IOP Publishing Ltd.

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1088/1742-6596/940/1/012028

Cite this

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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.",

author = "Tariq Al-Abdullah and D. Bemmerer and Z. Elekes and D. Schumann",

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AU - Bemmerer, D.

AU - Elekes, Z.

AU - Schumann, D.

PY - 2018/1/31

Y1 - 2018/1/31

N2 - 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.

AB - 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.

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DO - 10.1088/1742-6596/940/1/012028

M3 - Conference article

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