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相关论文: Neutrinophilic Non-Standard Interactions

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We present an $A_4$ flavor extended $\rm B-L$ model for realization of eV scale sterile neutrinos, motivated by the recent experimental hints from both particle physics and cosmology. The framework considered here is a gauged $\rm B-L$…

高能物理 - 唯象学 · 物理学 2020-06-24 Subhasmita Mishra , Mitesh Kumar Behera , Rukmani Mohanta , Sudhanwa Patra , Shivaramakrishna Singirala

Neutrino flavour oscillation is one of the primary indication of the existence of new physics beyond standard model. The presence of small neutrino mass is indispensable to explicate the oscillation among different flavours of neutrino. By…

高能物理 - 唯象学 · 物理学 2023-01-31 Trisha Sarkar

We introduce a model for Non-Standard neutral current Interaction (NSI) between neutrinos and the matter fields, with an arbitrary coupling to the up and down quarks. The model is based on a new $U(1)$ gauge symmetry with a light gauge…

高能物理 - 唯象学 · 物理学 2023-02-22 Nicolás Bernal , Yasaman Farzan

The phenomenon of neutrino oscillations has been established as the leading mechanism behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are massive and lepton flavors are mixed. Here we review…

高能物理 - 唯象学 · 物理学 2013-03-21 Tommy Ohlsson

Assuming dark matter to be asymmetric as well as self-interacting and neutrinos to be Dirac fermions, we propose a framework to address the observed baryon imbalance of the universe. We add three right-handed neutrinos…

高能物理 - 唯象学 · 物理学 2025-12-17 Manoranjan Dutta , Nimmala Narendra

We study a $U(1)_{B-L}$ extension of the Standard Model (SM) in which Dirac neutrino masses are generated radiatively at the one-loop level through the exchange of new beyond the SM fields. This framework establishes a direct connection…

高能物理 - 唯象学 · 物理学 2026-01-28 Chayan Majumdar , Utkarsh Patel , Supriya Senapati , Sudhanwa Patra

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…

高能物理 - 唯象学 · 物理学 2009-10-31 Sven Bergmann , Yuval Grossman

We explain the ATOMKI anomaly with a very light $Z'$ state that features non-anomalous and non-flavour-universal vector and axial-vector couplings to all leptons. This $Z'$ comes from a theoretical framework with a spontaneously broken…

高能物理 - 唯象学 · 物理学 2025-05-23 Rikard Enberg , Yaşar Hiçyılmaz , Stefano Moretti , Carlos Pérez de los Heros , Harri Waltari

In the presence of neutrino Non-Standard Interactions (NSI) with matter, the derivation of neutrino parameters from oscillation data must be reconsidered. In particular, along with the standard solution to neutrino oscillation, another…

高能物理 - 唯象学 · 物理学 2018-04-12 Peter B. Denton , Yasaman Farzan , Ian M. Shoemaker

Experimental hints for lepton-flavor universality violation in the muon's magnetic moment as well as neutral- and charged-current $B$-meson decays require Standard-Model extensions by particles such as leptoquarks that generically lead to…

高能物理 - 唯象学 · 物理学 2022-05-26 Julian Heeck , Anil Thapa

Discovering new neutrino interactions would provide evidence of physics beyond the Standard Model. We focus on flavor-dependent long-range neutrino interactions mediated by ultra-light mediators (masses below $10^{-10}$ eV) from…

高能物理 - 唯象学 · 物理学 2025-01-22 Masoom Singh , Mauricio Bustamante , Sanjib Kumar Agarwalla

We propose a new model with flavor-dependent gauged $U(1)_{B-L_1}\times U(1)_{B-L_{2}-L_{3}}$ symmetry in addition to the flavor-blind one in the standard model. The model contains three right-handed neutrinos to cancel gauge anomalies and…

高能物理 - 唯象学 · 物理学 2018-12-05 Linping Mu , Hiroshi Okada , Chao-Qiang Geng

We define a new class of Z' models with neutral flavour-changing interactions at tree level in the down-quark sector. They are related in an exact way to elements of the quark mixing matrix due to an underlying flavoured U(1)' gauge…

高能物理 - 唯象学 · 物理学 2016-06-30 Martin Jung

We study the flavor dependent $U(1)_{B_i-L_j}$ models, where an $i$th generation of quarks and $j(\neq i)$th generation of leptons are charged. By solving the anomaly free condition for the matter sector of the SM fermions and three…

高能物理 - 唯象学 · 物理学 2023-10-04 Nobuchika Okada , Osamu Seto

We consider a neutrinophilic $U(1)$ extension of the standard model (SM) which couples only to SM isosinglet neutral fermions, charged under the new group. The neutral fermions couple to the SM matter fields through Yukawa interactions. The…

高能物理 - 唯象学 · 物理学 2023-02-01 Waleed Abdallah , Anjan Kumar Barik , Santosh Kumar Rai , Tousik Samui

We investigate how neutrinos may acquire small electric charges within the Standard Model framework while preserving electromagnetic gauge invariance. Instead of gauging the standard hypercharge generator $Y$, a linear combination of $Y$…

高能物理 - 唯象学 · 物理学 2025-04-29 Sudip Jana , Michael Klasen , Vishnu P. K

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

The Standard Model's accidental and anomaly-free currents: $B-L$, $L_e-L_\mu$, $L_e-L_\tau$, and $L_\mu-L_\tau$, could be indicative of a hidden gauge structure beyond the Standard Model. Additionally, neutrino masses can be generated by a…

高能物理 - 唯象学 · 物理学 2016-02-23 Ryan Plestid

We review the status of the solutions to neutrino anomalies by flavor-changing as well as flavor-diagonal neutrino interactions. While it is difficult to explain the atmospheric neutrino data the solar neutrino data can be well accounted…

高能物理 - 唯象学 · 物理学 2009-10-31 Hiroshi Nunokawa

Model independent phenomenological studies, ranging from neutrino to B-physics, often consider effective interactions involving either purely vector (V), purely axial vector (A), or mixed vector and axial vector (V, A) couplings. While pure…

高能物理 - 唯象学 · 物理学 2026-03-31 Hemant Kumar Prajapati , Rahul Srivastava