Neutron-upscattering enhancement of the triple-alpha process

  • J. Bishop
  • , C. E. Parker
  • , G. V. Rogachev
  • , S. Ahn
  • , E. Koshchiy
  • , K. Brandenburg
  • , C. R. Brune
  • , R. J. Charity
  • , J. Derkin
  • , N. Dronchi
  • , G. Hamad
  • , Y. Jones-Alberty
  • , Tz Kokalova
  • , T. N. Massey
  • , Z. Meisel
  • , E. V. Ohstrom
  • , S. N. Paneru
  • , E. C. Pollacco
  • , M. Saxena
  • , N. Singh
  • R. Smith, L. G. Sobotka, D. Soltesz, S. K. Subedi, A. V. Voinov, J. Warren, C. Wheldon

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

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 12C, 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 CO2 gas, we measure the 3α-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).

Original languageEnglish
Article number2151
JournalNature communications
Volume13
Issue number1
DOIs
StatePublished - Dec 2022

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