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Phys. Rev. Lett. 85, 2909–2912 (2000)

Shape of the 8B Alpha and Neutrino Spectra

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C. E. Ortiz1, A. García1,2, R. A. Waltz1, M. Bhattacharya1,*, and A. K. Komives1
1University of Notre Dame, Notre Dame, Indiana 46556
2Lawrence Berkeley National Laboratory, Berkeley, California 94720

Received 15 March 2000; published in the issue dated 2 October 2000

The β-delayed α spectrum from the decay of 8B has been measured with a setup that minimized systematic uncertainties that affected previous measurements. Consequently the deduced neutrino spectrum presents much smaller uncertainties than the previous recommendation [J. N. Bahcall et al., Phys. Rev. C 54, 411 (1996)]. The 8B ν spectrum is found to be harder than previously recommended with about (10–20)% more neutrinos at energies between 12–14 MeV. The integrated cross sections of the 37Cl, 71Ga, 40Ar, and Super-Kamiokande detectors are, respectively, 3.6%, 1.4%, 5.7%, and 2.1% larger than previously thought.

© 2000 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.85.2909
DOI:
10.1103/PhysRevLett.85.2909
PACS:
23.40.Bw, 23.60.+e, 26.65.+t, 27.20.+n

*Present address: Nuclear Physics Laboratory, University of Washington, Seattle, WA 98195.