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Experimental study of resonant states in 27P via elastic scattering of 26Si+p

  • H. S. Jung*
  • , C. S. Lee
  • , Y. K. Kwon
  • , J. Y. Moon
  • , J. H. Lee
  • , C. C. Yun
  • , S. Kubono
  • , H. Yamaguchi
  • , T. Hashimoto
  • , D. Kahl
  • , S. Hayakawa
  • , Seonho Choi
  • , M. J. Kim
  • , Y. H. Kim
  • , Y. K. Kim
  • , J. S. Park
  • , E. J. Kim
  • , C. B. Moon
  • , T. Teranishi
  • , Y. Wakabayashi
  • N. Iwasa, T. Yamada, Y. Togano, S. Kato, S. Cherubini, G. G. Rapisarda
*Corresponding author for this work
  • Chung-Ang University
  • Institute for Basic Science
  • The University of Tokyo
  • Seoul National University
  • Hanyang University
  • Hoseo University
  • Kyushu University
  • Japan Atomic Energy Agency
  • Tohoku University
  • RIKEN
  • Yamagata University
  • National Institute for Nuclear Physics
  • University of Catania

Research output: Contribution to journalJournal articlepeer-review

Abstract

Proton resonant states in 27P were studied by the resonant elastic scattering of 26Si+p with a 26Si radioactive ion beam bombarding a thick H 2 gas target with the inverse kinematics method. The properties of these resonance states are important to better constrain the production rates of the 26Si(p,γ)27P reaction. This is one of the astrophysically important reactions needed to understand proton-rich nucleosynthesis such as the galactic production of 26Al and energy generation in explosive stellar environments. Although there are recent studies on the resonant structure in 27P, large uncertainties remain, and only a few levels are known. In this work, resonant states were observed over the excitation energies range of 2.3 to 3.8 MeV with high statistics and without background contamination within the target. The resonance parameters were extracted by an R-matrix analysis of the excitation function. The 26Si(p,γ)27P stellar reaction rate has been evaluated, including high-lying resonances found in this work.

Original languageEnglish
Article number045802
JournalPhysical Review C - Nuclear Physics
Volume85
Issue number4
DOIs
StatePublished - 2012.04.3

Quacquarelli Symonds(QS) Subject Topics

  • Physics & Astronomy

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