Astrophysical S(E) factor of 10B(p, α1)7Be at low energies.

Details Astrophysical S(E) factor of 10B(p, α1)7Be at low energies. Astrophysical S(E) factor of 10B(p, α1)7Be at low energies.

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993zphya.345..333a&link_type=abstract

Z. Phys., A, Vol. 345, No. 3, p. 333 - 334

Astronomy and Astrophysics

Astrophysics

3

Nuclear Reactions: Astrophysics

Scientific paper

The absolute cross section of the fusion reaction 10B(p, 4α1γ)7Be has been measured at the c.m. energy range E = 48 to 159 keV via the 429 keV secondary γ-ray transition. The studies involved high proton currents and thick solid 10B targets. The resulting cross sections have the same energy dependence as those of the 10B(p, α1)7Be reaction but they are lower by a factor 600.

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