Study of the <span class="aps-inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mi mathvariant="normal">Ca</mi></mrow><mrow><mn>48</mn></mrow></msup></mrow><mo>(</mo><mrow><msup><mrow><mi mathvariant="normal">He</mi></mrow><mrow><mn>3</mn></mrow></msup></mrow><mo>,</mo><mi> </mi><mi>p</mi><mo>)</mo><mrow><msup><mrow><mi mathvariant="normal">Sc</mi></mrow><mrow><mn>50</mn></mrow></msup></mrow></math></span> Reaction

H. Ohnuma; J. R. Erskine; J. A. Nolen, Jr; J. P. Schiffer; P. G. Roos

doi:10.1103/PhysRev.177.1695

Study of the ${Ca}^{48} ({He}^{3}, p) {Sc}^{50}$ Reaction

H. Ohnuma, J. R. Erskine, J. A. Nolen, Jr., J. P. Schiffer, and P. G. Roos

Phys. Rev. 177, 1695 – Published 20 January 1969

Abstract

The ${Ca}^{48} ({He}^{3}, p) {Sc}^{50}$ reaction was studied with a magnetic spectrograph at a bombarding energy of 12 MeV. Energy levels of ${Sc}^{50}$ were obtained. Spins and parities for these levels were assigned on the basis of a comparison between the experimental and calculated angular distributions. Distorted-wave Born-approximation theory and the shell-model wave functions due to Kuo and Brown were used to calculate the angular distributions.

Received 13 September 1968

DOI:https://doi.org/10.1103/PhysRev.177.1695

Authors & Affiliations

H. Ohnuma, J. R. Erskine, J. A. Nolen, Jr., and J. P. Schiffer

Argonne National Laboratory, Argonne, Illinois 60439

P. G. Roos

University of Maryland, College Park, Maryland

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Vol. 177, Iss. 4 — January 1969

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