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Experimental study of the Si30(He3,d)P31 reaction and thermonuclear reaction rate of Si30(p,γ)P31

D. S. Harrouz, N. de Séréville, P. Adsley, F. Hammache, R. Longland, B. Bastin, T. Faestermann, R. Hertenberger, M. La Cognata, L. Lamia, A. Meyer, S. Palmerini, R. G. Pizzone, S. Romano, A. Tumino, and H.-F. Wirth
Phys. Rev. C 105, 015805 – Published 14 January 2022

Abstract

Background: Abundance anomalies in some globular clusters, such as the enhancement of potassium and the depletion of magnesium, can be explained in terms of an earlier generation of stars polluting the presently observed ones. It was shown that the potential range of temperatures and densities of the polluting sites depends on the strength of a few critical reaction rates. The Si30(p,γ)P31 reaction has been identified as one of these important reactions.

Purpose: The key ingredient for evaluating the thermonuclear Si30(p,γ)P31 reaction rate is the strength of the resonances which, at low energy, are proportional to their proton width. Therefore, the goal of this work is to determine the proton widths of unbound P31 states.

Method: States in P31 were studied at the Maier-Leibnitz-Laboratorium using the one-proton Si30(He3,d)P31 transfer reaction. Deuterons were detected with the high resolution one quadrupole three dipoles (Q3D) magnetic spectrometer. Angular distribution and spectroscopic factors were extracted for 27 states, and proton widths and resonance strengths were calculated for the unbound states.

Results: Several P31 unbound states have been observed for the first time in a one-proton transfer reaction. Above 20 MK, the Si30(p,γ)P31 reaction rate is now entirely estimated from the observed properties of P31 states. The reaction rate uncertainty from all resonances other than the Erc.m.=149 keV resonance has been reduced down to less than a factor of 2 above that temperature. The unknown spin and parity of the Erc.m.=149 keV resonance dominates the uncertainty in the rate in the relevant temperature range.

Conclusion: The remaining source of uncertainty on the Si30(p,γ)P31 reaction rate comes from the unknown spin and parity of the Erc.m.=149 keV resonance which can change the reaction rate by a factor of 10 in the temperature range of interest.

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  • Received 16 July 2021
  • Accepted 21 December 2021

DOI:https://doi.org/10.1103/PhysRevC.105.015805

©2022 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

D. S. Harrouz1, N. de Séréville1,*, P. Adsley2,3,†, F. Hammache1, R. Longland4,5, B. Bastin6, T. Faestermann7, R. Hertenberger8, M. La Cognata9, L. Lamia9,10, A. Meyer1, S. Palmerini11,12, R. G. Pizzone9, S. Romano9,10,13, A. Tumino9,14, and H.-F. Wirth8

  • 1Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
  • 2School of Physics, University of the Witwatersrand, Johannesburg 2050, South Africa
  • 3iThemba Laboratory for Accelerator Based Sciences, Somerset West 7129, South Africa
  • 4North Carolina State University, Raleigh, North Carolina 27695, USA
  • 5Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708, USA
  • 6Grand Accélérateur National d'Ions Lourds (GANIL), CEA/DRF-CNRS/IN2P3, Boulevard Henri Becquerel, 14076 Caen, France
  • 7Physik Department E12, Technische Universität München, D-85748 Garching, Germany
  • 8Fakultät für Physik, Ludwig-Maximilians-Universität München, D-85748 Garching, Germany
  • 9Laboratori Nazionali del Sud–Istituto Nazionale di Fisica Nucleare, Via Santa Sofia 62, 95123 Catania, Italy
  • 10Dipartimento di Fisica e Astronomia E. Majorana, Università di Catania, 95131 Catania, Italy
  • 11Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, 06123 Perugia, Italy
  • 12Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, 06123 Perugia, Italy
  • 13Centro Siciliano di Fisica Nucleare e Struttura della Materia (CSFNSM), 95123 Catania, Italy
  • 14Facoltà di Ingegneria e Architettura, Università degli Studi di Enna, 94100 Enna, Italy

  • *nicolas.de-sereville@ijclab.in2p3.fr
  • Present address: Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA.

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Vol. 105, Iss. 1 — January 2022

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