Nature of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">Na</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>20</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math> 2646-keV level and the stellar reaction rate for <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">Ne</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>19</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math>(p,γ<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mo>)</mo></mrow><mrow><mn>20</mn></mrow></msup></mrow></math>Na

B. A. Brown; A. E. Champagne; H. T. Fortune; R. Sherr

doi:10.1103/PhysRevC.48.1456

Nature of the ${}^{20}{Na}$ 2646-keV level and the stellar reaction rate for ${}^{19}{Ne}$ (p,γ $)^{20}$ Na

B. A. Brown, A. E. Champagne, H. T. Fortune, and R. Sherr

Phys. Rev. C 48, 1456 – Published 1 September 1993

Abstract

Careful comparison of ${}^{20}F$ and ${}^{20}{Na}$ , and available data on reactions leading to both, suggests that $J^{π}$ (2646)= $3^{+}$ . Other mirror identifications are indicated and quantities of astrophysical interest are calculated.

Received 11 November 1992

DOI:https://doi.org/10.1103/PhysRevC.48.1456

Authors & Affiliations

B. A. Brown

Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824

A. E. Champagne

Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599
Triangle Universities Nuclear Laboratory, Duke University, Durham, North Carolina 27706

H. T. Fortune

Department of Physics, University of Pennsylvania, 209 S. 33rd Street, Philadelphia, Pennsylvania 19104

R. Sherr

Department of Physics, Princeton University, Princeton, New Jersey 08544

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Vol. 48, Iss. 3 — September 1993

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