The excitation function of the Al-27(alpha, n)P-30 reaction and its astrophysical application

Details The excitation function of the Al-27(alpha, n)P-30 reaction and its astrophysical application The excitation function of the Al-27(alpha, n)P-30 reaction and its astrophysical application

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phys...33..107h&link_type=abstract

Physica Scripta (ISSN 0031-8949), vol. 33, no. 2, Feb. 1986, p. 107-109.

Astronomy and Astrophysics

Astrophysics

2

Aluminum Isotopes, Astrophysics, Particle Energy, Phosphorus Isotopes, Reaction Kinetics, Thermonuclear Reactions, Solar System, Stellar Evolution, Synthesis (Chemistry), Temperature Gradients

Scientific paper

The yield from the Al-27(alpha, n)P-30 reaction from a thick Al-27 target is measured for alpha particles in the energy range from 3.04-3.66 eV, corresponding to stellar temperatures between 2.08 and 2.75 x 10 to the 9th K. The observed neutron yield curve is used to determine nucleosynthesis reaction rates. A value of 1.33 x 10 to the -22nd cu cm/mole/s is obtained and compared with results published elsewhere.

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