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

Arazi, A.; Faestermann, T.; Fernandez Niello, J.; Knie, K.; Korschinek, G.; Richter, E.; Rugel, G.; Wallner, C.

Abstract

Stellar nuclear reactions, generally occurring at energies well below the Coulomb barrier, have extremely low cross sections posing a very difficult task for theri determination using the usual promt gammy-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 strenghts of the 25Ma(p,gamma) reaction, by off-line counting of the produced 26Al nuclei.

Keywords: Nuclear reactions; Mass spectroscopy

  • New Astronomy Reviews 46 (2002) 525-528

Permalink: https://www.hzdr.de/publications/Publ-4833


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