Precise measurement of the ^7Be(p,gamma)^8B S-factor
arXiv:nucl-ex/0308003 · doi:10.1103/PhysRevC.68.065803
Abstract
We present new measurements of the ^7Be(p,gamma)^8B cross section from \bar{E}_{cm} = 116 to 2460 keV, that incorporate several improvements over our previously published experiment, also discussed here. Our new measurements lead to S_{17}(0) = 22.1 +- 0.6(expt) +- 0.6(theor) eV b based on data from \bar{E}_{cm} = 116 to 362 keV, where the central value is based on the theory of Descouvemont and Baye. The theoretical error estimate is based on the fit of 12 different theories to our low energy data. We compare our results to other S_{17}(0) values extracted from both direct (^7Be(p,gamma)^8B) and indirect (Coulomb dissociation and heavy-ion reaction) measurements, and show that the results of these 3 types of experiments are not mutually compatible. We recommend a "best" value, S_{17}(0) = 21.4 +- 0.5(expt) +- 0.6(theor) eV b, based on the mean of all modern direct measurements below the 1^+ resonance. We also present S-factors at 20 keV which is near the center of the Gamow window: the result of our measurements is S_{17}(20) = 21.4 +- 0.6(expt) +- 0.6(theor) eV b, and the recommended value is S_{17}(20) = 20.7 +- 0.5(expt) +- 0.6(theor) eV b.
22 pages, 20 figures
References in corpus (22)
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties
- Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data
- Solar Fusion Cross Sections
- How Uncertain Are Solar Neutrino Predictions?
- Solar Neutrinos Before and After KamLAND
- A Measurement of the Coulomb Dissociation of 8B at 254 MeV/nucleon and the 8B Solar Neutrino Flux
- New measurement and analysis of the 7Be(p,gamma)8B cross section
- Tests of Transfer Reaction Determinations of Astrophysical S-Factors
- 7Be(p,gamma)8B astrophysical S-factor from precision cross section measurements
- Study of the and capture reactions using the shell model embedded in the continuum
- A New Precision Measurement of the 7Be(p,gamma)8B Cross section with an Implanted 7Be Target
- Coulomb dissociation of 8B and the low-energy cross section of the 7Be(p,gamma)8B solar fusion reaction
- Low energy measurement of the 7Be(p,gamma)8B cross section
- S17(0) Determined from the Coulomb Breakup of 83 MeV/nucleon 8B
- Asymptotic normalization coefficients for 8B->7Be+p from a study of 8Li->7Li+n
- LMA MSW solution of the solar neutrino problem and first KamLAND results
- Asymptotic normalization coefficient of ^{8}B from breakup reactions and the S_{17} astrophysical factor
- A New Measurement of the Proton Capture Rate on 7Be and the S17(0) Factor
- Extrapolation of the astrophysical S factor for ^7Be(p,gamma)^8B to solar energies
- A new measurement of the 7Li(d,p)8Li cross section and consequences for 7Be(p,gamma)8B
- Measurement of Change of 7Be Decay Rate in Be and Au
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