1995
DOI: 10.1143/ptp.93.571
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Right-Handed b to c Coupling and CP Violation

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Cited by 6 publications
(7 citation statements)
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“…Furthermore, many extensions of the standard model predict new, effective four-Fermi interactions involving neutrinos, on which we will focus in this paper. General phenomenological studies of these non-standard interactions (NSIs) have been conducted in [1,2,3,4,5,6,7,8], and specific models are discussed in [9,10]. After a work by Grossman [11], which pointed out the importance of NSIs for neutrino oscillation experiments, many authors have investigated their impact in the context of solar neutrinos [12,13,14,15], atmospheric neutrinos [16,17,18,19,20,21], conventional and upgraded neutrino beams [22,23,24,25,26,27,28], neutrino factories [8,23,29,30,31,32,33,34], beta beams [35], supernova neutrinos [36,37], cosmological relic neutrinos [38], e + e − colliders [39], neutrino-electron scattering [40], and neutrino-nucleus scattering [41,42].…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, many extensions of the standard model predict new, effective four-Fermi interactions involving neutrinos, on which we will focus in this paper. General phenomenological studies of these non-standard interactions (NSIs) have been conducted in [1,2,3,4,5,6,7,8], and specific models are discussed in [9,10]. After a work by Grossman [11], which pointed out the importance of NSIs for neutrino oscillation experiments, many authors have investigated their impact in the context of solar neutrinos [12,13,14,15], atmospheric neutrinos [16,17,18,19,20,21], conventional and upgraded neutrino beams [22,23,24,25,26,27,28], neutrino factories [8,23,29,30,31,32,33,34], beta beams [35], supernova neutrinos [36,37], cosmological relic neutrinos [38], e + e − colliders [39], neutrino-electron scattering [40], and neutrino-nucleus scattering [41,42].…”
Section: Introductionmentioning
confidence: 99%
“…If we want to probe into such a tiny effect of NSI in the neutrino sector, extremely high sensitivities are required for experiments to detect deviations from the standard three flavor oscillations. A large number of papers in the literature is devoted to discuss NSI in various context including long-baseline accelerator experiments, the atmospheric and the solar neutrino observations, and supernova neutrinos [11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26].…”
Section: Introductionmentioning
confidence: 99%
“…[58]]. This contribution depends, for instance, on 23 . Since the leading atmospheric parameters cannot be determined precisely without near detectors (see above), there will be some use of the near detectors no matter if the flux is known or not, i.e., the cross section uncertainties will be translated into a background uncertainty.…”
Section: A Qualitative Discussionmentioning
confidence: 99%