New approach to determining radiative capture reaction rates at astrophysical energies
Name
PhysRevC.100.025804.pdf
Description
Published version
Size
4.66 MB
Format
Adobe PDF
Checksum (MD5)
94f5f4ceea2eaa23e1195b2070e4c086
Author(s)
Friščić, I
Donnelly, TW
Milner, RG
Date Issued
2019
Journal
Physical Review C
Publisher
American Physical Society (APS)
Version
Final published version
Abstract
© 2019 American Physical Society. Radiative capture reactions play a crucial role in stellar nucleosynthesis but have proved challenging to determine experimentally. In particular, the large uncertainty (≈100%) in the measured rate of the C12(α,γ)O16 reaction is the largest source of uncertainty in any stellar evolution model. With development of high-current energy-recovery linear accelerators (ERLs) and high-density gas targets, measurement of the O16(e,e′α)C12 reaction close to threshold using detailed balance allows a new approach to determine the C12(α,γ)O16 reaction rate with significantly increased precision (<20%). We present the formalism to relate photo- A nd electrodisintegration reactions and consider the design of an optimal experiment to deliver increased precision. Once the new ERLs come online, an experiment to validate the approach we propose should be carried out. This approach has broad applicability to radiative capture reactions in astrophysics.
MIT Department
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
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Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1103/PHYSREVC.100.025804
