6533b852fe1ef96bd12abd6c
RESEARCH PRODUCT
Precise Determination of the Unperturbed 8B Neutrino Spectrum
T. RogerJ. BüscherB. BastinOliver Sølund KirsebomR. RaabeM. AlcortaJ. ÄYstöM. J. G. BorgeM. Carmona-gallardoT. E. CocoliosJ. CruzP. DendoovenL. M. FraileH. O. U. FynboD. GalavizL. R. GasquesG. S. GiriM. HuyseS. HyldegaardK. JungmannW. L. KruithofM. LantzA. PereaK. RiisagerA. SaastamoinenB. SantraP. D. ShidlingM. SohaniA. J. SørensenO. TengbladE. TraykovD. J. Van Der HoekP. Van DuppenO. O. VersolatoH. W. Wilschutsubject
nuclear spectroscopyneutrino oscillationsPhysics::Instrumentation and Detectorsaccelerator-based physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]kiihdytinpohjainen fysiikkaKVIydinrakenne8Bnuclear structureydinspektroskopiaimplantationydinfysiikka23.40.Bw 26.65.+t 27.20.+nbeta-decaydescription
The measurement was performed at the Kernfysisch Versneller Instituut (KVI) at the University of Groningen, The Netherlands.; A measurement of the final state distribution of the 8B $\beta$ decay, obtained by implanting a 8B beam in a double-sided silicon strip detector, is reported here. The present spectrum is consistent with a recent independent precise measurement performed by our collaboration at the IGISOL facility, Jyvâskylä [O. S. Kirsebom et al., Phys. Rev. C 83, 065802 (2011)]. It shows discrepancies with previously measured spectra, leading to differences in the derived neutrino spectrum. Thanks to a low detection threshold, the neutrino spectrum is for the first time directly extracted from the measured final state distribution, thus avoiding the uncertainties related to the extrapolation of R-matrix fits. Combined with the IGISOL data, this leads to an improvement of the overall errors and the extension of the neutrino spectrum at high energy. The new unperturbed neutrino spectrum represents a benchmark for future measurements of the solar neutrino flux as a function of energy.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2012-04-01 |