AstrophysicalSFactor from Precision Cross Section Measurements
- 14 January 2002
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 88 (4) , 041101
- https://doi.org/10.1103/physrevlett.88.041101
Abstract
We measured the cross section from to 1200 keV, with a statistical-plus-systematic precision per point of better than . All important systematic errors were measured including backscattering losses. We obtain from our data at and the theory of Descouvemont and Baye.
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This publication has 24 references indexed in Scilit:
- Absolute cross section of 7Be(p,γ)8BNuclear Physics A, 2001
- Measurement of the Rate ofInteractions Produced bySolar Neutrinos at the Sudbury Neutrino ObservatoryPhysical Review Letters, 2001
- Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological PropertiesThe Astrophysical Journal, 2001
- Low-Energy Measurement of theCross SectionPhysical Review Letters, 2001
- How uncertain are solar neutrino predictions?Physics Letters B, 1998
- New Measurement and Analysis of theCross SectionPhysical Review Letters, 1998
- Proton capture cross section ofand the flux of high energy solar neutrinosPhysical Review C, 1983
- Study of the7be(p, γ)-reactionZeitschrift für Physik A Atoms and Nuclei, 1977
- Cross Sections for theReactionPhysical Review C, 1970
- ReactionPhysical Review B, 1966