Radiative neutrino mass generation: Models, flavour and the LHC

2017 ◽  
Vol 32 (14) ◽  
pp. 1742001
Author(s):  
Raymond R. Volkas
Keyword(s):  
Neutrino Mass ◽  
Lepton Number ◽  
Mass Generation ◽  
Low Energies ◽  
Mass Dimension ◽  
Flavour Violation ◽  
Neutrino Mass Generation ◽  
Neutrino Mass Models ◽  
Lepton Flavour

Radiative neutrino mass models and the seesaw models are viewed from the unifying framework of standard model effective operators that explicitly violate lepton number by two units [Formula: see text]. After some comments on naturalness and leptogenesis in the minimal type 1 seesaw model, a full list of minimal renormalisable models that produce mass dimension-7, [Formula: see text] operators at low energies is presented. By way of example, phenomenological bounds from Run 1 LHC and lepton flavour violation data are then placed on one of these models. A possible connection between radiative neutrino mass models and the current flavour anomalies in [Formula: see text] and [Formula: see text] transitions is then described.

scholarly journals A new mechanism of neutrino mass generation in the NMSSM with broken lepton number

2006 ◽  
Vol 642 (5-6) ◽  
pp. 503-509 ◽  
Author(s):  
Asmaa Abada ◽  
Gautam Bhattacharyya ◽  
Grégory Moreau
Keyword(s):  
Neutrino Mass ◽  
Lepton Number ◽  
Mass Generation ◽  
Neutrino Mass Generation

scholarly journals Searching for radiative neutrino mass generation at the LHC

2015 ◽  
Vol 30 (12) ◽  
pp. 1530030 ◽  
Author(s):  
Raymond R. Volkas
Keyword(s):  
Neutrino Mass ◽  
Explicit Model ◽  
Mass Generation ◽  
International Conference ◽  
Massive Neutrinos ◽  
Neutrino Mass Generation ◽  
Neutrino Mass Models ◽  
Lhc I

In this talk (talk given at the International Conference on Massive Neutrinos, Singapore, 9-13 February 2015), I describe the general characteristics of radiative neutrino mass models that can be probed at the LHC. I then cover the specific constraints on a new, explicit model of this type.

A modular A 4 symmetric scotogenic model for neutrino mass and dark matter

2021 ◽  
Author(s):  
Mitesh Kumar Behera ◽  
Shivaramakrishna Singirala ◽  
Subhasmita Mishra ◽  
R Mohanta
Keyword(s):  
Dark Matter ◽  
Neutrino Mass ◽  
Dirac Fermion ◽  
Dark Matter Candidate ◽  
Parameter Region ◽  
Mass Generation ◽  
Neutrino Mass Generation ◽  
Consistent Parameter ◽  
Radiative Mechanism ◽  
Lepton Flavour

Abstract Modular symmetries have been impeccable in neutrino and quark sectors. This motivated us, to propose a variant of scotogenic model based on modular $A_4$ symmetry and realize the neutrino mass generation at one-loop level through radiative mechanism. Alongside, we discuss the lepton flavour violating processes $\mu \to e \gamma$, $\mu \to3e$ and $\mu - e $ conversion in the nucleus. The lightest Dirac fermion turns out to be potential dark matter candidate, made stable by suitable assignment of modular weights. The relic density of the same has been computed with annihilations mediated by inert scalars and new $U(1)$ gauge boson. The LEP-II and ATLAS dilepton constraints on the new gauge parameters are suitably considered to show the consistent parameter region.

scholarly journals The hubble tension as a hint of leptogenesis and neutrino mass generation

2021 ◽  
Vol 81 (6) ◽  
Author(s):  
Miguel Escudero ◽  
Samuel J. Witte
Keyword(s):  
Neutrino Mass ◽  
Goldstone Boson ◽  
Predictive Distribution ◽  
Mass Generation ◽  
Posterior Predictive Distribution ◽  
Additional Energy ◽  
Dark Radiation ◽  
Neutrino Mass Generation ◽  
Neutrino Mass Models ◽  
The Universe

AbstractThe majoron, a neutrinophilic pseudo-Goldstone boson conventionally arising in the context of neutrino mass models, can damp neutrino free-streaming and inject additional energy density into neutrinos prior to recombination. The combination of these effects for an eV-scale mass majoron has been shown to ameliorate the outstanding $$H_0$$ H 0 tension, however only if one introduces additional dark radiation at the level of $$\Delta N_{\mathrm{eff}} \sim 0.5$$ Δ N eff ∼ 0.5 . We show here that models of low-scale leptogenesis can naturally source this dark radiation by generating a primordial population of majorons from the decays of GeV-scale sterile neutrinos in the early Universe. Using a posterior predictive distribution conditioned on Planck2018+BAO data, we show that the value of $$H_0$$ H 0 observed by the SH$$_0$$ 0 ES collaboration is expected to occur at the level of $$\sim 10\%$$ ∼ 10 % in the primordial majoron cosmology (to be compared with $$\sim 0.1\%$$ ∼ 0.1 % in the case of $$\Lambda $$ Λ CDM). This insight provides an intriguing connection between the neutrino mass mechanism, the baryon asymmetry of the Universe, and the discrepant measurements of $$H_0$$ H 0 .

scholarly journals Relaxing cosmological neutrino mass bounds with unstable neutrinos

2020 ◽  
Vol 2020 (12) ◽  
Author(s):  
Miguel Escudero ◽  
Jacobo Lopez-Pavon ◽  
Nuria Rius ◽  
Stefan Sandner
Keyword(s):  
Neutrino Mass ◽  
Particle Physics ◽  
Goldstone Boson ◽  
Mass Scale ◽  
Simple Extension ◽  
Type I ◽  
Mass Generation ◽  
Age Of The Universe ◽  
Neutrino Mass Models ◽  
The Right

Abstract At present, cosmological observations set the most stringent bound on the neutrino mass scale. Within the standard cosmological model (ΛCDM), the Planck collaboration reports ∑mv< 0.12 eV at 95 % CL. This bound, taken at face value, excludes many neutrino mass models. However, unstable neutrinos, with lifetimes shorter than the age of the universe τν ≲ tU, represent a particle physics avenue to relax this constraint. Motivated by this fact, we present a taxonomy of neutrino decay modes, categorizing them in terms of particle content and final decay products. Taking into account the relevant phenomenological bounds, our analysis shows that 2-body decaying neutrinos into BSM particles are a promising option to relax cosmological neutrino mass bounds. We then build a simple extension of the type I seesaw scenario by adding one sterile state ν4 and a Goldstone boson ϕ, in which νi→ ν4ϕ decays can loosen the neutrino mass bounds up to ∑mv ∼ 1 eV, without spoiling the light neutrino mass generation mechanism. Remarkably, this is possible for a large range of the right-handed neutrino masses, from the electroweak up to the GUT scale. We successfully implement this idea in the context of minimal neutrino mass models based on a U(1)μ−τ flavor symmetry, which are otherwise in tension with the current bound on ∑mv.

scholarly journals Testing radiative neutrino mass generation at the LHC

2007 ◽  
Vol 2007 (08) ◽  
pp. 022-022 ◽  
Author(s):  
Chian-Shu Chen ◽  
Chao-Qiang Geng ◽  
John N Ng ◽  
Jackson M.S Wu
Keyword(s):  
Neutrino Mass ◽  
Mass Generation ◽  
Neutrino Mass Generation

scholarly journals Exploding operators for Majorana neutrino masses and beyond

2021 ◽  
Vol 2021 (1) ◽  
Author(s):  
John Gargalionis ◽  
Raymond R. Volkas
Keyword(s):  
Neutrino Mass ◽  
Model Building ◽  
Dominant Role ◽  
New Physics ◽  
Majorana Neutrino ◽  
Effective Field ◽  
Tree Level ◽  
Mass Generation ◽  
Neutrino Mass Models ◽  
Almost All

Abstract Building UV completions of lepton-number-violating effective operators has proved to be a useful way of studying and classifying models of Majorana neutrino mass. In this paper we describe and implement an algorithm that systematises this model-building procedure. We use the algorithm to generate computational representations of all of the tree-level completions of the operators up to and including mass-dimension 11. Almost all of these correspond to models of radiative neutrino mass. Our work includes operators involving derivatives, updated estimates for the bounds on the new-physics scale associated with each operator, an analysis of various features of the models, and a look at some examples. We find that a number of operators do not admit any completions not also generating lower-dimensional operators or larger contributions to the neutrino mass, ruling them out as playing a dominant role in the neutrino-mass generation. Additionally, we show that there are at most five models containing three or fewer exotic multiplets that predict new physics that must lie below 100 TeV. Accompanying this work we also make available a searchable database containing all of our results and the code used to find the completions. We emphasise that our methods extend beyond the study of neutrino-mass models, and may be useful for generating completions of high-dimensional operators in other effective field theories. Example code: ref. [37].

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