# Ameliorating Higgs Induced Flavor Constraints on TeV Scale $W_R$

**Authors:** Rabindra N. Mohapatra, Guanwen Yan, Yongchao Zhang

arXiv: 1902.08601 · 2019-10-23

## TL;DR

This paper proposes an extension to the minimal left-right symmetric model to resolve flavor constraint tensions, predicts lower bounds on $W_R$ mass, and discusses implications for collider searches and dark matter models.

## Contribution

The paper introduces a scalar triplet extension to the LRSM that alleviates flavor constraints and predicts new $W_R$ decay modes, with testable mass bounds at the LHC.

## Key findings

- Lower bounds on $W_R$ mass range from 3.16 to 8.1 TeV depending on model parameters.
- The extended model predicts new decay modes of $W_R$ to two scalars.
- The model remains consistent with perturbativity and flavor constraints.

## Abstract

In the TeV scale minimal left-right symmetric model (LRSM) for neutrino masses, there is a tension between the flavor changing Higgs effects which prefer an $SU(2)_R$ breaking scale $v_R \gtrsim (15-25)$ TeV depending on whether the theory is kept invariant under charge conjugation ($Q_L\to (Q_R)^c$) or under parity ($Q_L\to Q_R$) respectively and an LHC accessible few-TeV range mass of $W_R$ boson which would require $v_R \lesssim 10 \, (15)$ TeV if $g_R/g_L = 1 (0.65)$. This requires one quartic coupling in the scalar potential to go non-perturbative, posing a theoretical problem if the $W_R$ is discovered at LHC. We propose a simple extension of the minimal LRSM that adds a $B-L=0$ scalar triplet and study how this can ameliorate this tension. We find that such a model is also constrained from various considerations and implies a lower bound on the $W_R$ mass of 8.1 (5.26) TeV for the parity case with $g_R/g_L= 1\, (0.65)$ and 4.85 (3.16) TeV for the case of charge conjugation, if the flavor constraints have to be avoided while keeping all couplings perturbative. These mass ranges are accessible at the high-luminosity LHC. The model also implies new decay mode of $W_R$ to two scalars which is absent in the minimal LRSM. Finally we comment on the impact of such a scalar multiplet for a class of dark matter extension of LRSM discussed in the literature recently.

## Full text

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## Figures

19 figures with captions in the complete paper: https://tomesphere.com/paper/1902.08601/full.md

## References

89 references — full list in the complete paper: https://tomesphere.com/paper/1902.08601/full.md

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Source: https://tomesphere.com/paper/1902.08601