Abstract
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 26β’πAlβ’(π,πΎ)β’27Si reaction to be 432+146β226ββmeV
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 26Al in astrophysical plasmas.
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 26Al in astrophysical plasmas.
| Original language | English |
|---|---|
| Article number | 042701 |
| Pages (from-to) | 1-6 |
| Number of pages | 6 |
| Journal | Physical Review Letters |
| Volume | 128 |
| Issue number | 4 |
| Early online date | 27 Jan 2022 |
| DOIs | |
| Publication status | Published - 28 Jan 2022 |
Fingerprint
Dive into the research topics of 'Radiative Capture on Nuclear Isomers: Direct Measurement of the 26β’πAlβ’(π,πΎ)β’27Si Reaction'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver