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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Format: | Government Document Electronic eBook |
Language: | English |
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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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245 | 0 | 0 | |a On the Normalization of the Neutrino Deuteron Cross Section |h [electronic resource] |
260 | |a Washington, D.C. : |b United States. Department of Energy. Office of High Energy Physics ; |a Oak Ridge, Tenn. : |b Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, |c 2001. | ||
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500 | |a 06/01/2001. | ||
500 | |a "FERMILAB-PUB-01-122-A." | ||
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500 | |a "arXiv:hep-ph/0106128." | ||
500 | |a "Other: oai:inspirehep.net:558293." | ||
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. | |
536 | |b AC02-07CH11359. | ||
650 | 7 | |a 72 physics of elementary particles and fields |2 local. | |
650 | 7 | |a Physics of elementary particles and fields |2 local. | |
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710 | 1 | |a United States. |b Department of Energy. |b Office of High Energy Physics. |4 spn. | |
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