Neutron-upscattering enhancement of the triple-alpha process
The neutron inelastic scattering of carbon-12, populating the Hoyle state, is a reaction of interest for the triple-alpha process. The inverse process (neutron upscattering) can enhance the Hoyle state’s decay rate to the bound states of 12 C, effectively increasing the overall triple-alpha reaction rate. The cross section of this reaction is impossible to measure experimentally but has been determined here at astrophysically-relevant energies using detailed balance. Using a highly-collimated monoenergetic beam, here we measure neutrons incident on the Texas Active Target Time Projection Chamber (TexAT TPC) filled with CO 2 gas, we measure the 3 α -particles (arising from the decay of the Hoyle state following inelastic scattering) and a cross section is extracted. Here we show the neutron-upscattering enhancement is observed to be much smaller than previously expected. The importance of the neutron-upscattering enhancement may therefore not be significant aside from in very particular astrophysical sites (e.g. neutron star mergers).
- Research Organization:
- Ohio University, Athens, OH (United States); Texas A & M University, College Station, TX (United States); Washington University, St. Louis, MO (United States)
- Sponsoring Organization:
- National Science Foundation (NSF); Nuclear Solutions Institute; Science and Technology Facilities Council (STFC); USDOE; USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC)
- Grant/Contract Number:
- FG02-87ER40316; FG02-88ER40387; FG02-93ER40773; NA0003841; NA0003883; NA0003909; SC0019042
- OSTI ID:
- 1864069
- Alternate ID(s):
- OSTI ID: 1904601
- Journal Information:
- Nature Communications, Journal Name: Nature Communications Journal Issue: 1 Vol. 13; ISSN 2041-1723
- Publisher:
- Nature Publishing GroupCopyright Statement
- Country of Publication:
- United Kingdom
- Language:
- English
Similar Records
Experiments to Further the Understanding of the Triple-Alpha Process in Hot Astrophysical Scenarios