Low-energy cross section of theBe7(p,γ)B8solar fusion reaction from the Coulomb dissociation ofB8-Reference-Cited by-同舟云学术

Low-energy cross section of theBe7(p,γ)B8solar fusion reaction from the Coulomb dissociation ofB8

Published:2006-01-27 Issue:1 Volume:73 Page:
ISSN:0556-2813
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Schümann F.,Typel S.,Hammache F.,Sümmerer K.,Uhlig F.,Böttcher I.,Cortina D.,Förster A.,Gai M.,Geissel H.,Greife U.,Grosse E.,Iwasa N.,Koczoń P.,Kohlmeyer B.,Kulessa R.,Kumagai H.,Kurz N.,Menzel M.,Motobayashi T.,Oeschler H.,Ozawa A.,Płoskoń M.,Prokopowicz W.,Schwab E.,Senger P.,Strieder F.,Sturm C.,Sun Zhi-Yu,Surówka G.,Wagner A.,Waluś W.

Publisher

American Physical Society (APS)

Subject

Nuclear and High Energy Physics

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.73.015806/fulltext

Reference40 articles.

1. Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

2. Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters

3. Electron energy spectra, fluxes, and day-night asymmetries of8B solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino Observatory

4. What Do We (Not) Know Theoretically about Solar Neutrino Fluxes?

5. Surprising Sun: A New Step Towards a Complete Picture?

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