208Pb(n, γ) Cross Sections by Activation between 10 and 200 keV

Details 208Pb(n, γ) Cross Sections by Activation between 10 and 200 keV 208Pb(n, γ) Cross Sections by Activation between 10 and 200 keV

May 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrv..181.1639m&link_type=abstract

Physical Review, vol. 181, Issue 4, pp. 1639-1642

Physics

3

Scientific paper

The 208Pb(n, γ)209Pb activation cross section has been measured in the energy range relevant to stellar nucleosynthesis. A large-area, low-background β-ray counting system was developed to obtain sufficient sensitivity. Information on the radiative widths of the known resonances below 120 keV was derived. The cross-section average found for the Maxwellian temperature distribution assumed for a stellar interior (kT=30 keV) is 13 mb. This value is quite compatible with expectations based on current nucleosynthesis theory.

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