# Bounds on heavy Majorana neutrinos in type-I seesaw and implications for   collider searches

**Authors:** Arindam Das, Nobuchika Okada

arXiv: 1702.04668 · 2018-03-21

## TL;DR

This paper investigates the parameter space of heavy Majorana neutrinos in the type-I seesaw model, considering experimental constraints, and discusses prospects for collider detection at future high-energy colliders.

## Contribution

It provides a comprehensive parameter scan of heavy Majorana neutrinos in the minimal seesaw model, incorporating multiple experimental constraints and highlighting future collider search potentials.

## Key findings

- Heavy neutrino mixings are more constrained than current LHC limits.
- Allowed parameter regions can be probed at HL-LHC and future 100 TeV colliders.
- Parameter space consistent with neutrino data and precision measurements is identified.

## Abstract

The neutrino masses and flavor mixings, which are missing in the Standard Model (SM), can be naturally incorporated in the type-I seesaw extension of the SM with heavy Majorana neutrinos being singlet under the SM gauge group. If the heavy Majorana neutrinos are around the electroweak scale and their mixings with the SM neutrinos are sizable, they can be produced at high energy colliders, leaving characteristic signatures with lepton-number violations. Employing the general parametrization for the neutrino Dirac mass matrix in the minimal seesaw scenario, we perform a parameter scan and identify allowed regions to satisfy a variety of experimental constraints from the neutrino oscillation data, the electroweak precision measurements and the lepton-flavor violating processes. We find that the resultant mixing parameters between the heavy neutrinos and the SM neutrinos are more severely constrained than those obtained from the current search for heavy Majorana neutrinos at the LHC. Such parameter regions can be explored at the High-Luminosity LHC and a 100 TeV pp-collider in the future.

## Full text

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## Figures

34 figures with captions in the complete paper: https://tomesphere.com/paper/1702.04668/full.md

## References

83 references — full list in the complete paper: https://tomesphere.com/paper/1702.04668/full.md

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Source: https://tomesphere.com/paper/1702.04668