Indirect experimental approaches to reactions important for stellar hydrogen burning

Details Indirect experimental approaches to reactions important for stellar hydrogen burning Indirect experimental approaches to reactions important for stellar hydrogen burning

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..529..434i&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: 10th International Symposium. AIP Conference Proceedings, Volume 529, pp. 43

Astronomy and Astrophysics

Astrophysics

Hydrostatic Stellar Nucleosynthesis, Radiative Capture, X- And Gamma-Ray Spectroscopy, 20<=A<=38

Scientific paper

A large number of proton capture reactions cannot be measured directly at astrophysically important energies with current experimental techniques. Over the past decade, indirect methods have been used extensively for the study of nuclear structure and nuclear reaction mechanisms in order to infer the nuclear cross sections of astrophysical interest. Some of the experimental techniques will be discussed by using as an example a recent study of the 24Mg(p,γ)25Al reaction which is important for hydrogen burning in globular cluster red giant stars. .

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