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It is by now established that neutrino oscillations occur due to non-zero masses and parameters in the leptonic mixing matrix. The extraction of oscillation parameters may be complicated due to subleading effects such as non-standard…

高能物理 - 唯象学 · 物理学 2016-08-03 Mehedi Masud , Poonam Mehta

The possible non-standard interactions (NSIs) of neutrinos with matter plays important role in the global determination of neutrino properties. In our study we select various data sets from LHC measurements at 13 TeV with integrated…

高能物理 - 唯象学 · 物理学 2021-02-24 DianYu Liu , ChuanLe Sun , Jun Gao

We investigate source and detector non-standard neutrino interactions at the proposed ESS$\nu$SB experiment. We analyze the effect of non-standard physics at the probability level, the event-rate level and by a full computation of the…

高能物理 - 唯象学 · 物理学 2015-09-29 Mattias Blennow , Sandhya Choubey , Tommy Ohlsson , Sushant K. Raut

We propose several Two Higgs Doublet Models with the addition of an Abelian gauge group which free the usual framework from flavor changing neutral interactions and explain neutrino masses through the seesaw mechanism. We discuss the…

高能物理 - 唯象学 · 物理学 2017-09-13 Miguel D. Campos , D. Cogollo , Manfred Lindner , T. Melo , Farinaldo S. Queiroz , Werner Rodejohann

We discuss the possible implications of physics beyond the standard model in the neutrino sector applying non-standard interaction. Recently, the NOvA and T2K neutrino experiments have announced their measurements for the CP violating…

高能物理 - 唯象学 · 物理学 2025-04-01 Anjan Giri

The neutrino oscillation experiments are setting increasingly strong upper bounds on the vector Non-Standard neutrino Interactions (NSI) with matter fields. However, the bounds on the axial NSI are more relaxed, raising the hope that…

高能物理 - 唯象学 · 物理学 2025-08-12 S. Abbaslu , Yasaman Farzan

Theories beyond the Standard Model must respect its gauge symmetry. This implies strict constraints on the possible models of Non-Standard Neutrino Interactions (NSIs). We review here the present status of NSIs from the point of view of…

高能物理 - 唯象学 · 物理学 2009-11-26 D. Hernandez

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

Current neutrino experiments measure the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of experiments will be sensitive to subdominant effects that can give information on the unknown neutrino…

高能物理 - 唯象学 · 物理学 2018-01-30 Y. Farzan , M. Tortola

We study a modified version of the Standard Model that includes a scalar doublet and two right-handed neutrinos, forming the neutrinophillic two higgs doublet ($\nu\text{2HDM}$) framework. For $v_2 << v_1$, this model operates at a TeV…

高能物理 - 唯象学 · 物理学 2025-05-30 Abhishek , V. Suryanarayana Mummidi

The limitations of the Standard Model in explaining neutrino masses and neutrino mixing lead to the exploration of frameworks beyond the Standard Model (BSM). The possibility of neutrinos interacting with fermions via a scalar mediator is…

高能物理 - 唯象学 · 物理学 2024-12-31 Moon Moon Devi , Dharitree Bezboruah , Abinash Medhi , Arnab Sarker , Debajyoti Dutta

We explore the possibility of probing the nonstandard interactions between the neutrino and a hypothetical massive scalar or pseudoscalar via neutrino flavor transformation in supernovae. We find that in the ultrarelativistic limit, the…

高能天体物理现象 · 物理学 2018-06-06 Yue Yang , James P. Kneller

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…

高能物理 - 唯象学 · 物理学 2025-01-16 Qiu-Xia Yi , Ya-Ru Wang , Shu-Jun Rong

One of the primary objectives of Deep Underground Neutrino Experiment (DUNE) is to discover the leptonic CP violation and to identify it's source. In this context, we study the impact of non-standard neutrino interactions (NSIs) on…

高能物理 - 唯象学 · 物理学 2018-10-17 K. N. Deepthi , Srubabati Goswami , Newton Nath

We discuss the sensitivity reach of a neutrino factory measurement to non-standard neutrino interactions (NSI), which may exist as a low-energy manifestation of physics beyond the Standard Model. We use the muon appearance mode \nu_e -->…

高能物理 - 唯象学 · 物理学 2009-01-06 N. Cipriano Ribeiro , H. Minakata , H. Nunokawa , S. Uchinami , R. Zukanovich Funchal

Neutrino non-standard interactions (NSI) play a crucial role in neutrino oscillations and can provide valuable insights for constructing models of neutrino masses and mixing. While NSI have been widely explored through oscillation and…

高能物理 - 唯象学 · 物理学 2025-07-16 Sudip Jana , Saumyen Kundu , Santosh Kumar Rai

Non-Standard Interactions (NSI) of neutrinos may originate from models in which new particles interact with neutrinos. In scalar extensions of the SM, the typical approach to obtain NSI requires Fierz transformations and charged Higgses,…

高能物理 - 唯象学 · 物理学 2018-11-14 Ingolf Bischer , Werner Rodejohann , Xun-Jie Xu

General Neutrino Interactions (GNI) are scalar, pseudoscalar, vector, axial vector or tensor interactions of neutrinos with fermions, and generalise the often studied neutrino Non-Standard Interactions (NSI). If GNI arise from heavy new…

高能物理 - 唯象学 · 物理学 2019-09-05 Ingolf Bischer , Werner Rodejohann

Neutrino non-standard interactions (NSI), previously introduced for the sun, are studied in the supernova context. For normal hierarchy the probability for electron neutrinos and antineutrinos at low energy ($E\lesssim 0.8-0.9 MeV$) is…

高能物理 - 唯象学 · 物理学 2013-04-10 C. R. Das , Joao Pulido

Recently, there has been a growing interest in extensions of the Standard Model in which naturally small Dirac neutrino masses arise due to existence of a symmetry which protects neutrino's Diracness. Motivated by this, we consider an…

高能物理 - 唯象学 · 物理学 2019-12-11 S. S. Correia , R. G. Felipe , F. R. Joaquim