Physics – Nuclear Physics
Scientific paper
Oct 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..dnp..b406b&link_type=abstract
American Physical Society, Division of Nuclear Physics Meeting, October 28-31, 1998 Santa Fe, New Mexico, abstract #B4.06
Physics
Nuclear Physics
Scientific paper
Proton radiative capture on ^14N is the slowest reaction in the CN-cycle. Therefore, in a massive main sequence star whose energy is generated primarily through the CN-cycle, this reaction has the role of setting the energy generation rate for the star and consequently the time scale for its evolution. In addition, the rate of the ^14N(p,γ)^15O reaction is a significant variable in the width of the globular cluster age distribution derived from computer models of stellar evolution. The lower limit of this distribution is thought to be a firm estimate for the lower limit on the age of the universe. The extrapolation of existing S-factor data down to stellar energies is complicated by interference effects from the 6.79 MeV subthreshold level in ^15O. The situation could be improved by a direct determination of the mean lifetime of this state. We have attempted such a measurement using the Doppler Shift Attenuation Method (DSAM). Results and implications will be presented.
Bertone P. F.
Champagne Arthur E.
Iliadis Ch.
Powell Denise C.
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