How Accurately Do We Know the Cross Section of the 7Be(p, γ)8B Reaction?

Details How Accurately Do We Know the Cross Section of the 7Be(p, γ)8B Reaction? How Accurately Do We Know the Cross Section of the 7Be(p, γ)8B Reaction?

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..819..171g&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: 12th International Symposium. AIP Conference Proceedings, Volume 819, pp. 17

Astronomy and Astrophysics

Astrophysics

3

Radiative Capture, 6<=A<=19, Fundamental Aspects Of Astrophysics, Solar Neutrinos, Particle Emission, Solar Wind

Scientific paper

The ``world average'' of the astrophysical cross section factor , S17(0), is driven by the Seattle result due to the very small quoted uncertainty, which we however demonstrate it to be an overestimated accuracy. We propose more realistic error bars for the Seattle results based on the published Seattle data. This leads to a an uncertainty of the measured slope of S17 and thus an uncertainty due to extrapolation that can be reasonably estimated to be -3.0+0.0 eV-b.

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