On the Normalization of the Neutrino Deuteron Cross Section [electronic resource]

As is well-known, comparison of the solar neutrino fluxes measured in SuperKamiokande (SK) by $\nu + ê- \to \nu + ê-$ and in the Sudbury Neutrino Observatory (SNO) by $\nu_e + d \to ê- + p + p$ can provide a ̀̀smoking gun'' signature for neutrino oscillations as the solution to the sola...

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Bibliographic Details
Online Access: Full Text (via OSTI)
Corporate Author: Fermi National Accelerator Laboratory (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : United States. Department of Energy. Office of High Energy Physics ; Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 2001.
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MARC

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500 |a Beacom, John F. ; Parke, Stephen J. ;  
520 3 |a As is well-known, comparison of the solar neutrino fluxes measured in SuperKamiokande (SK) by $\nu + ê- \to \nu + ê-$ and in the Sudbury Neutrino Observatory (SNO) by $\nu_e + d \to ê- + p + p$ can provide a ̀̀smoking gun'' signature for neutrino oscillations as the solution to the solar neutrino puzzle. This occurs because SK has some sensitivity to all active neutrino flavors whereas SNO can isolate electron neutrinos. This comparison depends crucially on the normalization and uncertainty of the theoretical charged-current neutrino-deuteron cross section. We address a number of effects which are significant enough to change the interpretation of the SK--SNO comparison. 
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