New Precision Measurement of theCross Section
- 29 December 2004
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 93 (26) , 262503
- https://doi.org/10.1103/physrevlett.93.262503
Abstract
The reaction plays an important role in determining the high energy solar neutrino flux and in understanding the abundances of primordial . This Letter reports a new precision measurement of the cross sections of this direct capture reaction, determined by measuring the ensuing activity in the region of to 950 keV. Various recent theoretical fits to our data result in a consistent extrapolated value of .
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This publication has 33 references indexed in Scilit:
- What Do We (Not) Know Theoretically about Solar Neutrino Fluxes?Physical Review Letters, 2004
- Precise measurement of thefactorPhysical Review C, 2003
- New measurement of the proton capture rate onand thefactorPhysical Review C, 2003
- Coulomb Dissociation ofand the Low-Energy Cross Section of theSolar Fusion ReactionPhysical Review Letters, 2003
- Precision Measurement of theCross Section with an ImplantedTargetPhysical Review Letters, 2003
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino ObservatoryPhysical Review Letters, 2002
- AstrophysicalSFactor from Precision Cross Section MeasurementsPhysical Review Letters, 2002
- Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological PropertiesThe Astrophysical Journal, 2001
- Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino DataPhysical Review Letters, 2001
- Radiativeα-capture cross sections from realistic nucleon-nucleon interactions and variational Monte Carlo wave functionsPhysical Review C, 2001