Lotay G, Lennarz A, Ruiz C, Akers C, Chen A A, Christian G, Connolly D, Davids B, Davinson T, Fallis J, Hutcheon D A, Machule P, Martin L, Mountford D J, Murphy A St J
Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom.
TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
Phys Rev Lett. 2022 Jan 28;128(4):042701. doi: 10.1103/PhysRevLett.128.042701.
We present the first direct measurement of an astrophysical reaction using a radioactive beam of isomeric nuclei. In particular, we have measured the strength of the key 447-keV resonance in the ^{26m}Al(p,γ)^{27}Si reaction to be 432_{-226}^{+146} meV and find that this resonance dominates the thermally averaged reaction rate for temperatures between 0.3 and 2.5 GK. This work represents a critical development in resolving one of the longest standing issues in nuclear astrophysics research, relating to the measurement of proton capture reactions on excited quantum levels, and offers unique insight into the destruction of isomeric ^{26}Al in astrophysical plasmas.
我们展示了首次使用同质异能核的放射性束对天体物理反应进行的直接测量。具体而言,我们测量了(^{26m}Al(p,γ)^{27}Si)反应中关键的447 keV共振强度为(432_{-226}^{+146}) meV,并发现该共振在0.3至2.5 GK的温度范围内主导了热平均反应速率。这项工作代表了解决核天体物理学研究中最长期存在的问题之一的关键进展,该问题与激发量子能级上质子俘获反应的测量有关,并为天体物理等离子体中同质异能(^{26}Al)的破坏提供了独特的见解。