2020
DOI: 10.1103/physrevd.101.055047
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Borexino and general neutrino interactions

Abstract: We derive constraints on all possible general neutrino-electron interactions (scalar, vector, pseudo-scalar, axial-vector and tensor) using the recent real time Borexino event rate measurements of pp, pep and 7 Be solar neutrinos. Some of the limits improve from TEXONO and CHARM-II for incoming electron and muon neutrinos while the rest remains weaker for Borexino and those for the tau flavor are the first ones. Future improvements by next-generation solar neutrino experiments are also studied. The limits exte… Show more

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Cited by 45 publications
(36 citation statements)
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“…For larger masses, y φee is constrained by tests of the inverse-square law of gravity [57,58], the Casimir effect [59], stellar cooling processes [60,61], N eff in cosmology [62][63][64][65][66], supernovae [67][68][69][70][71][72][73], neutrino scattering [74][75][76][77][78][79], etc. But all these bounds are significantly higher than the largest expected values of y φee -see ref.…”
Section: Phenomenologymentioning
confidence: 99%
“…For larger masses, y φee is constrained by tests of the inverse-square law of gravity [57,58], the Casimir effect [59], stellar cooling processes [60,61], N eff in cosmology [62][63][64][65][66], supernovae [67][68][69][70][71][72][73], neutrino scattering [74][75][76][77][78][79], etc. But all these bounds are significantly higher than the largest expected values of y φee -see ref.…”
Section: Phenomenologymentioning
confidence: 99%
“…We thus take into account the constraints from the CHARM-II experiment [23,24] as well as reactor neutrino using TEXONO [25] data. The relevant data were used to study the electromagnetic interactions or the nonstandard vector-type interactions of a neutrino via the transition νe → νe [26][27][28][29][30][31]. The heavy neutral leptons as well as DM scattering off electrons can be also searched in high-energy neutrino beam-dump experiment or far-forward detector at the LHC [32,33].…”
Section: Jhep05(2021)131mentioning
confidence: 99%
“…The four-fermion operators are analogous to those in ref. [31]. Here the dimensionless parameters M α , E α , a α and˜ a α are in general complex.…”
Section: The General Neutrino Interactions With Exotic Fermion Via Neutrinoelectron Scatteringmentioning
confidence: 99%
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“…The solar neutrino spectrum measured by Borexino in Phase II of the experimental program [27] gives us control over the e-NSI through EνES, while the COHERENT collaboration's open data release and observation of the CEνNS interaction at a CsI detector [28] provides sensitivity to the u and d quark NSI. Analyses have been performed with these data sets in both minimal NSI scenarios and for a broad range of operators [5,[29][30][31][32][33][34][35], but to explore the full space of NSI degeneracies we will allow an NSI set of maximum size to be free to vary, which has not been done before. Secondly, the stopped-pion spallation neutrino source (SNS) at COHERENT only produces ν e , ν µ , andν µ neutrinos, and with a short baseline to the detectors, there is negligible oscillation of the neutrino flux into τ flavors.…”
Section: Combining Oscillation Ceνns and Eνes Datamentioning
confidence: 99%