Constraining {sup 26}Al+{ital p} resonances using {sup 26}Al({sup 3}He,{ital d}){sup 27}Si
- W. K. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125 (United States)
- Department of Physics, Princeton University, Princeton, New Jersey 08544 (United States)
- A. W. Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06511 (United States)
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)
The {sup 26}Al({sup 3}He,{ital d}){sup 27}Si reaction was measured from 0{degree}{le}{theta}{sub c.m.}{le}35{degree} at {ital E}({sup 3}He)=20 MeV using a quadrupole-dipole-dipole-dipole magnetic spectrometer. States in {sup 27}Si were observed above the background at 7652 and 7741 keV and upper limits were set for the state at 7592 keV. Implications for the {sup 26}Al({ital p},{gamma}){sup 27}Si stellar reaction rate are discussed. {copyright} {ital 1996 The American Physical Society.}
- OSTI ID:
- 282157
- Journal Information:
- Physical Review, C, Journal Name: Physical Review, C Journal Issue: 4 Vol. 53; ISSN 0556-2813; ISSN PRVCAN
- Country of Publication:
- United States
- Language:
- English
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