First inverse kinematics measurement of resonances in Be7(α,γ)C11 relevant to neutrino-driven wind nucleosynthesis using DRAGON

A. Psaltis, A. A. Chen, R. Longland, D. S. Connolly, C. R. Brune, B. Davids, J. Fallis, R. Giri, U. Greife, D. A. Hutcheon, L. Kroll, A. Lennarz, J. Liang, M. Lovely, M. Luo, C. Marshall, S. N. Paneru, A. Parikh, C. Ruiz, A. C. Shotter, and M. Williams
Phys. Rev. C 106, 045805 – Published 14 October 2022

Abstract

A possible mechanism to explain the origin of the light p nuclei in the Galaxy is the nucleosynthesis in the proton-rich neutrino-driven wind ejecta of core-collapse supernovas via the νp process. However, this production scenario is very sensitive to the underlying supernova dynamics and the nuclear physics input. As far as the nuclear uncertainties are concerned, the breakout from the pp chains via the Be7(α,γ)C11 reaction has been identified as an important link which can influence the nuclear flow and, therefore, the efficiency of the νp process. However, its reaction rate is poorly known over the relevant temperature range, T = 1.5–3 GK. We report on the first direct measurement of two resonances of the Be7(α,γ)C11 reaction with previously unknown strengths using an intense radioactive Be7 beam from the Isotope Separator and Accelerator (ISAC-I) Center facility and the DRAGON recoil separator in inverse kinematics. We have decreased the Be7(α,γ)C11 reaction rate uncertainty to 9.410.7% over the relevant temperature region.

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  • Received 31 December 2021
  • Revised 1 July 2022
  • Accepted 12 September 2022

DOI:https://doi.org/10.1103/PhysRevC.106.045805

©2022 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

A. Psaltis1,2,*, A. A. Chen1,2, R. Longland3,4, D. S. Connolly5,†, C. R. Brune6, B. Davids5,7, J. Fallis8, R. Giri6, U. Greife9, D. A. Hutcheon5, L. Kroll1,2, A. Lennarz5, J. Liang1,‡, M. Lovely9, M. Luo10, C. Marshall3,4,§, S. N. Paneru6,∥, A. Parikh11, C. Ruiz5,12, A. C. Shotter13, and M. Williams5,14

  • 1Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
  • 2The NuGrid Collaboration, https://nugrid.github.io/
  • 3Department of Physics, North Carolina State University, Raleigh, North Carolina 27695, USA
  • 4Triangle Universities Nuclear Laboratory, Duke University, Durham, North Carolina 27710, USA
  • 5TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
  • 6Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
  • 7Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
  • 8North Island College, 2300 Ryan Road, Courtenay, British Columbia V9N 8N6, Canada
  • 9Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
  • 10Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
  • 11Department de Física, Universitat Politècnica de Catalunya, E-08036 Barcelona, Spain
  • 12Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8W 2Y2, Canada
  • 13School of Physics, University of Edinburgh EH9 3JZ Edinburgh, United Kingdom
  • 14Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom

  • *Present address: Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany; psaltisa@mcmaster.ca
  • Present address: Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA.
  • Present address: TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • §Present address: Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA.
  • Facility for Rare Isotope Beams, East Lansing, Michigan 48824, USA.

See Also

Direct Measurement of Resonances in Be7(α,γ)C11 Relevant to νp-Process Nucleosynthesis

A. Psaltis, A. A. Chen, R. Longland, D. S. Connolly, C. R. Brune, B. Davids, J. Fallis, R. Giri, U. Greife, D. A. Hutcheon, L. Kroll, A. Lennarz, J. Liang, M. Lovely, M. Luo, C. Marshall, S. N. Paneru, A. Parikh, C. Ruiz, A. C. Shotter, and M. Williams
Phys. Rev. Lett. 129, 162701 (2022)

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Vol. 106, Iss. 4 — October 2022

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