Measurement of the 25Mg(p,γ)26Al reaction at stellar energies

Details Measurement of the 25Mg(p,γ)26Al reaction at stellar energies Measurement of the 25Mg(p,γ)26Al reaction at stellar energies

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002newar..46..525a&link_type=abstract

New Astronomy Reviews, Volume 46, Issue 8-10, p. 525-528.

Astronomy and Astrophysics

Astronomy

4

Scientific paper

Stellar nuclear reactions, generally occurring at energies well below the Coulomb barrier, have extremely low cross sections posing a very difficult task for their determination using the usual prompt γ-ray detection method. We describe here the application of the highly sensitive Accelerator Mass Spectrometry technique (AMS) as an alternative method for the determination of the resonance strengths of the 25Mg(p,γ) reaction, by off-line counting of the produced 26Al nuclei.

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