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相关论文: Viable models for large non-standard neutrino inte…

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Nonstandard neutrino interactions (NSI) arising from light and heavy mediators probe different sectors of the parameter space of models focusing on phenomena that require the extension of the standard model. High-energy scattering…

高能物理 - 唯象学 · 物理学 2023-06-28 Timo J. Kärkkäinen , Zoltán Trócsányi

Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore,…

高能物理 - 唯象学 · 物理学 2016-12-07 Charles J. Stapleford , Daavid J. Väänänen , James P. Kneller , Gail C. McLaughlin , Brandon T. Shapiro

We present a simple extension of the Standard Model that leads to renormalizable long-range vector-mediated neutrino self-interactions. This model can resolve the Hubble tension by delaying the onset of neutrino free-streaming during…

高能物理 - 唯象学 · 物理学 2020-12-04 Maximilian Berbig , Sudip Jana , Andreas Trautner

We investigate non-standard neutrino interactions (NSIs) in the triplet seesaw model featuring non-trivial correlations between NSI parameters and neutrino masses and mixing parameters. We show that sizable NSIs can be generated as a…

高能物理 - 唯象学 · 物理学 2009-02-18 Michal Malinsky , Tommy Ohlsson , He Zhang

The SuperKamiokande atmospheric neutrino measurements leave substantial room for nonstandard interactions (NSI) of neutrinos with matter in the nu_e- nu_tau sector. Large values of the NSI couplings are accommodated if the vacuum…

高能物理 - 唯象学 · 物理学 2009-11-11 Alexander Friedland , Cecilia Lunardini

The triplet scalars $(\Delta=\Delta^{++},\Delta^{+},\Delta^{0})$, utilized in the so-called Type-II seesaw model to explain the lightness of neutrinos, would generate nonstandard interactions (NSI) for neutrino propagating in matter. We…

高能物理 - 唯象学 · 物理学 2018-06-06 Katri Huitu , Timo J. Kärkkäinen , Jukka Maalampi , Sampsa Vihonen

We present perturbative oscillation probabilities for electron and muon channels including non-standard interaction (NSI) effects. The perturbation was performed in standard parameters $\Delta m^2_{21}/\Delta m^2_{31}$ and…

高能物理 - 唯象学 · 物理学 2020-11-30 Mariano Esteves Chaves , Diego Rossi Gratieri , Orlando Luis Goulart Peres

We present a detailed analysis of a class of extensions to the SM Gauge chiral symmetry $SU(3)_{C}\times SU(3)_{L}\times U(1)_{X}$ (331 model), where the neutrino electroweak interaction with matter via charged and neutral current is…

高能物理 - 唯象学 · 物理学 2011-08-29 M. Medina , P. C. de Holanda

Neutrino oscillation experiments in the past decades have greatly improved our knowledge on neutrinos by measuring the fundamental neutrino parameters. The ongoing and upcoming neutrino oscillation experiments are intended to pin down the…

高能物理 - 唯象学 · 物理学 2013-07-16 Tommy Ohlsson , He Zhang , Shun Zhou

Future dark matter (DM) direct detection searches will be subject to irreducible neutrino backgrounds that will challenge the identification of an actual WIMP signal in experiments without directionality sensitivity. We study the impact of…

高能物理 - 唯象学 · 物理学 2017-12-29 D. Aristizabal Sierra , N. Rojas , M. H. G. Tytgat

We construct UV-complete models for non-standard neutrino interactions mediated by a sub-GeV gauge boson Z' coupled to baryon number $B$ or $B-L$. A flavor-dependent Z' coupling to neutrinos is induced by mixing a U(1)'-charged Dirac…

高能物理 - 唯象学 · 物理学 2016-09-22 Yasaman Farzan , Julian Heeck

The neutrino experiments utilize heavy nuclear targets to achieve high statistics neutrino-nucleus interaction event rate, which leads to systematic uncertainties in the oscillation parameters due to the nuclear effects and uncertainties in…

高能物理 - 唯象学 · 物理学 2024-10-07 R Lalnuntluanga , R K Pradhan , A Giri

We consider effects of the Non-Standard Interactions (NSI) on oscillations of the high energy atmospheric neutrinos. The \nu_\mu-oscillograms are constructed and their dependence on the NSI strength parameters \epsilon_{\alpha \beta}…

高能物理 - 唯象学 · 物理学 2015-06-15 Arman Esmaili , Alexei Yu. Smirnov

We examine the MiniBooNE neutrino, MiniBooNE antineutrino and LSND antineutrino data sets in a two-neutrino $\stackrel{\tiny{(-)}}{\nu}_{\mu}\rightarrow\stackrel{\tiny{(-)}}{\nu}_e$ oscillation approximation subject to non-standard matter…

高能物理 - 唯象学 · 物理学 2012-02-07 G. Karagiorgi , M. H. Shaevitz , J. M. Conrad

Unmodeled beyond Standard Model (BSM) physics in neutrino propagation can masquerade as parameter degeneracies in future precision measurements. Because the upcoming DUNE and T2HK experiments will operate at substantially different…

高能物理 - 唯象学 · 物理学 2026-03-17 João Paulo Pinheiro , Ushak Rahaman

The implementation of seesaw mechanisms to give mass to neutrinos in the presence of an anomaly-free U(1)_X gauge symmetry is discussed in the context of minimal extensions of the standard model. It is shown that type-I and type-III seesaw…

高能物理 - 唯象学 · 物理学 2010-04-23 D. Emmanuel-Costa , Edison T. Franco , R. Gonzalez Felipe

Motivated by the recent Super-Kamiokande results on atmospheric neutrinos, we incorporate massive neutrinos, with large angle oscillation between the second and third generations, in a scenario with R-parity violating supersymmetry. We…

高能物理 - 唯象学 · 物理学 2009-10-31 Biswarup Mukhopadhyaya , Sourov Roy , Francesco Vissani

Neutrino oscillations have become well-known phenomenon; the measurements of neutrino mixing angles and mass squared differences are continuously improving. Future oscillation experiments will eventually determine the remaining unknown…

高能物理 - 唯象学 · 物理学 2015-09-30 O. G. Miranda , H. Nunokawa

Precision measurements of neutrino oscillation parameters have provided a tremendous boost to the search for sub-leading effects due to several beyond the Standard Model scenarios in neutrino oscillation experiments. Among these, two of the…

高能物理 - 唯象学 · 物理学 2023-05-29 Sadashiv Sahoo , Anil Kumar , Sanjib Kumar Agarwalla , Amol Dighe

In this work, we investigate the implications of a novel non-standard interaction (NSI) of neutrinos. This interaction is geometric in origin -- it arises because the propagation of fermions in curved spacetime induces torsion. This torsion…

高能物理 - 唯象学 · 物理学 2026-02-10 Riya Barick , Indrajit Ghose , Srubabati Goswami , Amitabha Lahiri , Sushant K. Raut