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APS » Journals » Phys. Rev. C » Volume 53 » Issue 4
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Phys. Rev. C 53, 1945–1949 (1996)

Constraining 26Al+p resonances using 26Al(3He,d)27Si

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R. B. Vogelaar, L. W. Mitchell, and R. W. Kavanagh
W. K. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125

A. E. Champagne
Department of Physics, Princeton University, Princeton, New Jersey 08544

P. V. Magnus, M. S. Smith, A. J. Howard, and P. D. Parker
A. W. Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06511

H. A. O’Brien
Los Alamos National Laboratory, Los Alamos, New Mexico 87545

Received 1 November 1995; published in the issue dated April 1996

The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipole-dipole-dipole magnetic spectrometer. States in 27Si were observed above the background at 7652 and 7741 keV and upper limits were set for the state at 7592 keV. Implications for the 26Al(p,γ)27Si stellar reaction rate are discussed. © 1996 The American Physical Society.

© 1996 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.53.1945
DOI:
10.1103/PhysRevC.53.1945
PACS:
25.55.Hp, 26.20.+f, 27.30.+t
 
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