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Related papers: Probing non-standard neutrino-electron interaction…

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Neutrino-electron scattering experiments play a crucial role in investigating the non-standard interactions of neutrinos. In certain models, these interactions can include interference terms that may affect measurements. Next-generation…

High Energy Physics - Phenomenology · Physics 2023-05-19 Jong-Chul Park , Gaurav Tomar

We explore the effects of nonstandard neutrino interactions in the lower components of the solar neutrino spectrum which are predominant by the vacuum oscillations. The recent measurements of Borexino experiment between 2011 and 2015…

High Energy Physics - Phenomenology · Physics 2017-09-29 Amir N. Khan , Douglas W. McKay

Many extensions of the Standard Model lead to non-standard neutrino interactions (NSI), which can affect the interpretation of current and future neutrino data. We explore an alternative approach to the study of these dimension eight four…

High Energy Physics - Phenomenology · Physics 2013-05-29 Sacha Davidson , Veronica Sanz

Constraints on couplings of several Beyond Standard Model Physics scenarios, mediated by massive intermediate particles including (1) Extra Z-prime, (2) New Light Spin-1 Boson, and (3) Charged Higgs Boson, are placed via neutrino-electron…

High Energy Physics - Phenomenology · Physics 2018-03-28 B. Sevda , A. Şen , M. Demirci , M. Deniz , M. Agartioglu , A. Ajjaq , S. Kerman , L. Singh , A. Sonay , H. T. Wong , M. Zeyrek

For standard neutrinos, recent solar neutrino results together with the assumption of a nuclearly powered Sun imply severe constraints on the individual components of the total neutrino flux: \Phi_{Be}<0.7*10^9cm^-2 s^-1, \Phi_{CNO}<…

We report the results of a study of electroweak parameters from observations of neutral-current $\nu$N deeply inelastic scattering in the CCFR detector at the FNAL Tevatron Quadrupole Triplet neutrino beam. An improved extraction of the…

High Energy Physics - Experiment · Physics 2007-05-23 K. S. McFarland

We suggest a would-be solution to the solar neutrino tension why solar neutrinos appear to mix differently from reactor antineutrinos, in theoretical respect. To do that, based on an extended theory with light sterile neutrinos added we…

High Energy Physics - Phenomenology · Physics 2021-03-31 Y. H. Ahn

The recently reported astrophysical neutrinos events in the TeV-PeV energy range open a winder to explore new physics at energy frontiers. In this paper, we examine effects of non-standard interactions (NSIs) on the PeV neutrinos events. We…

High Energy Physics - Phenomenology · Physics 2025-01-16 Qiu-Xia Yi , Ya-Ru Wang , Shu-Jun Rong

We propose a new \emph{CPT}-even and Lorentz-violating nonminimal coupling between fermions and Abelian gauge fields involving the CPT-even tensor $(K_{F})_{\mu\nu\alpha\beta}$ of the standard model extension. We thus investigate its…

High Energy Physics - Theory · Physics 2012-12-27 R. Casana , M. M. Ferreira , R. V. Maluf , F. E. P. dos Santos

We investigate the implications of non-standard interactions on neutrino oscillations in the OPERA experiment. In particular, we study the non-standard interaction parameter $\epsilon_{\mu\tau}$. We show that the OPERA experiment has a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mattias Blennow , Davide Meloni , Tommy Ohlsson , Francesco Terranova , Mattias Westerberg

We reexamine the constraints on mixing between electron and muon or tau neutrinos from shock-reheating and r-process nucleosynthesis in supernovae. To this end neutrino flavor evolution is described by nonlinear equations following from a…

Astrophysics · Physics 2009-10-22 G. Sigl

The neutral-current (NC) non-standard interactions (NSI) of neutrinos with fermions can modify the flavor oscillations of atmospheric neutrinos as they propagate through the Earth. We present constraints on the NC-NSI parameters…

High Energy Physics - Phenomenology · Physics 2025-12-30 J Krishnamoorthi , Anil Kumar , Sanjib Kumar Agarwalla

We discuss physics of the three neutrino flavor transformation with non-unitary mixing matrix, with particular attention to the correlation between the $\nu$SM- and the $\alpha$ parameters which represent effect of unitarity violating (UV)…

High Energy Physics - Phenomenology · Physics 2020-05-20 Ivan Martinez-Soler , Hisakazu Minakata

Cosmological observations are becoming increasingly sensitive to the effects of light particles in the form of dark radiation (DR) at the time of recombination. The conventional observable of effective neutrino number, $N_{\rm eff}$, is…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-30 Christopher Brust , Yanou Cui , Kris Sigurdson

The Standard Model (SM) of particle physics effectively explains most observed phenomena, though some anomalies, especially in the neutrino sector, suggest the need for extensions. In this Letter, we perform the first global fit of elastic…

High Energy Physics - Phenomenology · Physics 2025-12-05 Mattia Atzori Corona , Matteo Cadeddu , Nicola Cargioli , Francesca Dordei , Carlo Giunti , Christoph A. Ternes

We explore the impact of nonstandard interactions on neutrino propagation in accretion disks around binary neutron star mergers remnants. We show flavor evolution can be significantly modified even for values of the nonstandard couplings…

High Energy Physics - Phenomenology · Physics 2018-02-14 Amélie Chatelain , Maria Cristina Volpe

It is well-known that in addition to the standard LMA solution to solar anomaly, there is another solution called LMA-Dark which requires Non-Standard Interactions (NSI) with effective couplings as large as the Fermi coupling. Although this…

High Energy Physics - Phenomenology · Physics 2015-08-26 Yasaman Farzan

We show that non-standard neutrino self-interactions can lead to total flavor equipartition in a dense neutrino gas, such as those expected in core-collapse supernovae. In this first investigation of this phenomenon in the multi-angle…

High Energy Astrophysical Phenomena · Physics 2023-05-17 Sajad Abbar

Solar and KamLAND data are in slight tension when interpreted in the standard two-flavor oscillations framework and this may be alleviated allowing for a non-zero value of the mixing angle theta_13. Here we show that, likewise, non-standard…

High Energy Physics - Phenomenology · Physics 2009-12-01 A. Palazzo , J. W. F. Valle

If the atmospheric and the solar neutrino problem are both explained by neutrino oscillations, and if there are only three light neutrinos, then all mass-squared differences between the neutrinos are known. In such a case, existing…

High Energy Physics - Phenomenology · Physics 2009-10-31 Sven Bergmann , Yuval Grossman
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