Gravitational Wave imprints of the Doublet Left-Right Symmetric Model

Fuente: arXiv
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Main Authors: Karmakar, Siddhartha, Ringe, Dhruv
Format: Preprint
Published: 2023
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author Karmakar, Siddhartha
Ringe, Dhruv
author_facet Karmakar, Siddhartha
Ringe, Dhruv
contents We study the gravitational wave (GW) signature in the doublet left-right symmetric model (DLRSM) resulting from the strong first-order phase transition (SFOPT) associated with $SU(2)_R\times U(1)_{B-L}$-breaking. For different values of the symmetry-breaking scale $v_R =20,~30$, and $50$ TeV, we construct the one-loop finite temperature effective potential to explore the parameter space for regions showing SFOPT. We identify the region where the associated stochastic GW background is strong enough to be detected at planned GW observatories. A strong GW background favors a relatively light neutral CP-even scalar $H_{3}$, arising from the $SU(2)_R$ doublet. The $SU(2)_L$ subgroup of DLRSM is broken by three vevs: $κ_1,~κ_2$, and $v_L$. We observe a preference for $\mathcal{O}(1)$ values of the ratio $w=v_L/κ_1$, but no clear preference for the ratio $r=κ_2/κ_1$. A large number of points with strong GW background can be ruled out from precise measurement of the trilinear Higgs coupling and searches for $H_3$ at future colliders.
format Preprint
id arxiv_https___arxiv_org_abs_2309_12023
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Gravitational Wave imprints of the Doublet Left-Right Symmetric Model
Karmakar, Siddhartha
Ringe, Dhruv
High Energy Physics - Phenomenology
We study the gravitational wave (GW) signature in the doublet left-right symmetric model (DLRSM) resulting from the strong first-order phase transition (SFOPT) associated with $SU(2)_R\times U(1)_{B-L}$-breaking. For different values of the symmetry-breaking scale $v_R =20,~30$, and $50$ TeV, we construct the one-loop finite temperature effective potential to explore the parameter space for regions showing SFOPT. We identify the region where the associated stochastic GW background is strong enough to be detected at planned GW observatories. A strong GW background favors a relatively light neutral CP-even scalar $H_{3}$, arising from the $SU(2)_R$ doublet. The $SU(2)_L$ subgroup of DLRSM is broken by three vevs: $κ_1,~κ_2$, and $v_L$. We observe a preference for $\mathcal{O}(1)$ values of the ratio $w=v_L/κ_1$, but no clear preference for the ratio $r=κ_2/κ_1$. A large number of points with strong GW background can be ruled out from precise measurement of the trilinear Higgs coupling and searches for $H_3$ at future colliders.
title Gravitational Wave imprints of the Doublet Left-Right Symmetric Model
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2309.12023