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In these lecture notes we present mechanisms for the generation of Majorana neutrino masses and lepton mixing. We consider simple extensions of the Standard Model. Apart from a section about radiative mass generation, we put special…

高能物理 - 唯象学 · 物理学 2009-01-06 W. Grimus

A new idea for neutrino mass was proposed recently, where its smallness is not due to the seesaw mechanism, i.e. not inversely proportional to some large mass scale. It comes from a one-loop mechanism with dark matter in the loop consisting…

高能物理 - 唯象学 · 物理学 2013-06-06 Subhaditya Bhattacharya , Ernest Ma , Alexander Natale , Ahmed Rashed

Recently, several reactor oscillation experiments have successively measured a nonzero value for the neutrino mixing angle ${\theta_{13}}$, which is greater than 5 standard deviations. Within framework of the $\mu$ from $\nu$ Supersymmetric…

高能物理 - 唯象学 · 物理学 2013-08-23 Hai-Bin Zhang , Tai-Fu Feng , Li-Na Kou , Shu-Min Zhao

We consider a version of the low-scale type I seesaw mechanism for generating small neutrino masses, as an alternative to the standard seesaw scenario. It involves two right-handed (RH) neutrinos $\nu_{1R}$ and $\nu_{2R}$ having a Majorana…

高能物理 - 唯象学 · 物理学 2018-04-27 J. T. Penedo , S. T. Petcov , Tsutomu T. Yanagida

We provide a comprehensive analysis of the Type-I Seesaw family of neutrino mass models, including the conventional type-I seesaw and its low-scale variants, namely the linear and inverse seesaws. We establish that all these models…

高能物理 - 唯象学 · 物理学 2025-11-17 Salvador Centelles Chuliá , Antonio Herrero-Brocal , Avelino Vicente

We provide a list of particle physics models at the TeV-scale that are compatible with neutrino masses and dark matter. In these models, the Standard Model particle content is extended with a small number (\leq 4) of scalar and fermion…

高能物理 - 唯象学 · 物理学 2015-06-16 Diego Restrepo , Oscar Zapata , Carlos Yaguna

We discuss various physics aspects of neutrino oscillation with non-standard interactions (NSI). We formulate a perturbative framework by taking \Delta m^2_{21} / \Delta m^2_{31}, s_{13}, and the NSI elements \epsilon_{\alpha \beta}…

高能物理 - 唯象学 · 物理学 2009-03-27 Takashi Kikuchi , Hisakazu Minakata , Shoichi Uchinami

Non-Standard neutral current Interactions (NSIs) of neutrinos with matter can alter the pattern of neutrino oscillation due to the coherent forward scattering of neutrinos on the medium. This effect makes long-baseline neutrino experiments…

高能物理 - 唯象学 · 物理学 2016-08-03 Yasaman Farzan , Ian M. Shoemaker

Scalar Non-Standard Interactions (SNSI) in neutrinos can arise when a scalar mediator couples to both neutrinos and standard model fermions. This beyond the Standard Model (BSM) scenario is particularly interesting as the SNSI contribution…

高能物理 - 唯象学 · 物理学 2024-10-08 Dharitree Bezboruah , Dibya S. Chattopadhyay , Abinash Medhi , Arnab Sarker , Moon Moon Devi

Neutrino masses can be generated by fermion triplets with TeV-scale mass, that would manifest at LHC as production of two leptons together with two heavy SM vectors or higgs, giving rise to final states such as 2 leptons + 4 jets (that can…

高能物理 - 唯象学 · 物理学 2008-11-26 Roberto Franceschini , Thomas Hambye , Alessandro Strumia

Contrary to the common lore based on naive dimensional analysis, the seesaw scale for neutrino masses can be naturally in the TeV range, with small parameters coming from radiative corrections. We present one such class of type-I seesaw…

高能物理 - 唯象学 · 物理学 2015-08-03 P. S. Bhupal Dev , Chang-Hun Lee , R. N. Mohapatra

Next generation direct dark matter (DM) detection experiments will have unprecedented capabilities to explore coherent neutrino-nucleus scattering (CE$\nu$NS) complementary to dedicated neutrino experiments. We demonstrate that future DM…

高能物理 - 唯象学 · 物理学 2024-12-03 Thomas Schwemberger , Volodymyr Takhistov , Tien-Tien Yu

We consider a class of models in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector. In this framework, the light neutrinos are partially…

高能物理 - 唯象学 · 物理学 2021-03-16 Zackaria Chacko , Patrick J. Fox , Roni Harnik , Zhen Liu

We study the phenomenology of a Standard Model (SM) extension with two charged singlet scalars and three right handed (RH) neutrinos at an electron-positron collider. In this model, the neutrino mass is generated radiatively at three-loop,…

高能物理 - 唯象学 · 物理学 2014-05-13 Amine Ahriche , Salah Nasri , Rachik Soualah

If there exist only three light neutrinos below the weak scale, the neutrino masses can arise by breaking the lepton number L. One example is the Zee mechanism for the neutrino masses. We study phenomenological implications of neutrino…

高能物理 - 唯象学 · 物理学 2007-05-23 Jihn E. Kim , Jae Sik Lee

We study neutrino mass generation within the framework of non-holomorphic modular symmetry proposed by Qu and Ding. In this formalism, neutrino masses are generated via the Type-I seesaw mechanism, where the Yukawa couplings depend on…

高能物理 - 唯象学 · 物理学 2026-04-21 Cheshta , Priya , Suneel Dutt , B. C. Chauhan

Radiative seesaw models are examples of interesting and testable extensions of the Standard Model to explain the light neutrino masses. In radiative models at 1-loop level, such as the popular scotogenic model, in order to successfully…

Monojet events at colliders have been used to probe models of dark matter and extra dimensions. We point out that these events also probe extensions of the Standard Model modifying neutrino-quark interactions. Such nonstandard interactions…

高能物理 - 唯象学 · 物理学 2012-07-31 Alexander Friedland , Michael L. Graesser , Ian M. Shoemaker , Luca Vecchi

We discuss the simplest mechanisms for generating neutrino masses at tree level and one loop level. We find a significant number of new possibilities where one can generate neutrino masses at the one-loop level by adding only two new types…

高能物理 - 唯象学 · 物理学 2009-09-09 Pavel Fileviez Perez , Mark B. Wise

We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Esteban-Pretel , R. Tomàs , J. W. F. Valle