A New Precision Measurement of the 7Be(p,gamma)8B Cross section with an Implanted 7Be Target
arXiv:nucl-ex/0208005 · doi:10.1103/PhysRevLett.90.022501
Abstract
The 7Be(p,gamma)8B reaction plays a central role in the evaluation of solar neutrino fluxes. We report on a new precision measurement of the cross section of this reaction, following our previous experiment with an implanted 7Be target, a raster scanned beam and the elimination of the backscattering loss. The new measurement incorporates a more abundant 7Be target and a number of improvements in design and procedure. The point at Elab=991 keV was measured several times under varying conditions, yielding a value of S17(Ec.m. =850 keV) = 24.0(5) eV b. Measurements were carried out at lower energies as well. Due to the precise knowledge of the implanted 7Be density profile it was possible to reconstitute both the off- and on resonance parts of the cross section and to obtain from the entire set of measurements an extrapolated value of S17(0)=21.2(7) eV b.
4 Pages, 3 Figures
References in corpus (11)
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data
- Solar Fusion Cross Sections
- Where do we stand with solar neutrino oscillations?
- 7Be(p,gamma)8B astrophysical S-factor from precision cross section measurements
- Unknowns after the SNO Charged-Current Measurement
- Low energy measurement of the 7Be(p,gamma)8B cross section
- Solar Neutrinos: Probing the Quasi-Isothermal Solar Core Produced by SUSY Dark Matter Particles
- A new measurement of the 7Li(d,p)8Li cross section and consequences for 7Be(p,gamma)8B
- What have we learnt about the Sun from the measurement of the B neutrino flux?
Cited by in corpus (46)
- Solar fusion cross sections II: the pp chain and CNO cycles
- What do we (not) know theoretically about solar neutrino fluxes?
- Solar Neutrinos: Status and Prospects
- Solar models with accretion. I. Application to the solar abundance problem
- Unified ab initio approaches to nuclear structure and reactions
- Solar models and solar neutrino oscillations
- Odd-even mass differences from self-consistent mean-field theory
- Effective field theory description of halo nuclei
- Radiative capture of nucleons at astrophysical energies with single-particle states
- A New Precision Measurement of the 3He(4He,gamma)7Be Cross section
- Ab initio many-body calculation of the 7Be(p,gamma)8B radiative capture
- Precise measurement of the ^7Be(p,gamma)^8B S-factor
- Coulomb dissociation of 8B and the low-energy cross section of the 7Be(p,gamma)8B solar fusion reaction
- Asymptotic normalization coefficients for 8B->7Be+p from a study of 8Li->7Li+n
- Electromagnetic Dissociation as a Tool for Nuclear Structure and Astrophysics
- The Impact of Recent Advances in Laboratory Astrophysics on our Understanding of the Cosmos
- Low-energy cross section of the 7Be(p,g)8B solar fusion reaction from Coulomb dissociation of 8B
- A New Measurement of the Proton Capture Rate on 7Be and the S17(0) Factor
- Halo effective field theory constrains the solar Beryllium-7 + proton -> Boron-8 + photon rate
- Electromagnetic dissociation of 8B and the astrophysical S factor for 7Be(p,gamma)8B
- 7Be(p,gamma)8B S-factor from ab initio no-core shell model wave functions
- Description of the proton and neutron radiative capture reactions in the Gamow shell model
- Marrying ab initio calculations and Halo EFT: the case of
- Precision Measurement of the Decay Rate of 7Be in Host Materials
- 7Be(p,gamma)8B S-factor from ab initio wave functions
- Analysis of Coulomb breakup experiments of 8B with a dynamical eikonal approximation
- Solar Models and Solar Neutrinos: Current Status
- Low-lying non-normal parity states in 8B measured by proton elastic scattering on 7Be
- Constraining Low-Energy Proton Capture on Beryllium-7 through Charge Radius Measurements
- Nuclear processes in Astrophysics: Recent progress
- Ab initio informed evaluation of the radiative capture of protons on Be
- Solar fusion III: New data and theory for hydrogen-burning stars
- Solar Hydrogen Burning and Neutrinos
- Models, measurements, and effective field theory: proton capture on Beryllium-7 at next-to-leading order
- Asymptotic normalization coefficients for from the peripheral (,) reaction and their astrophysical application
- Constraining the Be()B -factor with the new precise Be solar neutrino flux from Borexino
- Asymptotic normalization coefficients (nuclear vertex constants) for and the direct astrophysical S-factors at solar energies
- Astrophysical S factor and rate of direct capture reaction in a potential model
- Rotating Solar Models in Agreement with Helioseismic Results and Updated Neutrino Fluxes
- Coupled-channels treatment of in effective field theory
- Low-Energy Nuclear Astrophysics - the Fascinating Region of A=7
- Solar Fusion and The Coulomb Dissociation of 8B; What Have We Learned and Where Do We Go From Here?
- Structure of B and astrophysical factor
- A study of the fine-structure constant dependence of radiative capture in Halo-EFT
- Status of the Standard Solar Model Prediction of Solar Neutrino Fluxes
- The Coulomb Dissociation of 8B and a Critical Assessment of the Seattle S17(0) Result