CERN Accelerating science

Article
Report number arXiv:2308.12804 ; PITT-PACC-2317 ; IP/BBSR/2023-09
Title Searching for heavy leptophilic Z′: from lepton colliders to gravitational waves
Related titleSearching for Heavy Leptophilic $Z'$: from Lepton Colliders to Gravitational Waves
Author(s) Dasgupta, Arnab (Pittsburgh U.) ; Dev, P S Bhupal (McDonnell Ctr. Space Sci.) ; Han, Tao (Pittsburgh U.) ; Padhan, Rojalin (Pittsburgh U. ; Bhubaneswar, Inst. Phys. ; HBNI, Mumbai) ; Wang, Si (Pittsburgh U.) ; Xie, Keping (Pittsburgh U. ; Michigan State U.)
Publication 2023
Imprint 2023-08-24
Number of pages 51
In: JHEP 2312 (2023) 011
DOI 10.1007/JHEP12(2023)011 (publication)
Subject category hep-ph ; astro-ph.CO ; hep-ex ; Particle Physics - Phenomenology ; Astrophysics and Astronomy ; Particle Physics - Experiment
Study IMCC
Abstract We study the phenomenology of leptophilic $Z'$ gauge bosons at the future high-energy $e^+e^-$ and $\mu^+\mu^-$ colliders, as well as at the gravitational wave observatories. The leptophilic $Z'$ model, although well-motivated, remains largely unconstrained from current low-energy and collider searches for $Z'$ masses above ${\cal O}(100 {\rm GeV})$, thus providing a unique opportunity for future lepton colliders. Taking $U(1)_{L_\alpha-L_\beta} (\alpha,\beta=e,\mu,\tau)$ models as concrete examples, we show that future $e^+e^-$ and $\mu^+\mu^-$ colliders with multi-TeV center-of-mass energies provide unprecedented sensitivity to heavy leptophilic $Z'$ bosons. Moreover, if these $U(1)$ models are classically scale-invariant, the phase transition at the $U(1)$ symmetry-breaking scale tends to be strongly first-order with ultra-supercooling, and leads to observable stochastic gravitational wave signatures. We find that the future sensitivity of gravitational wave observatories, such as advanced LIGO-VIRGO and Cosmic Explorer, can be complementary to the collider experiments, probing higher $Z'$ masses up to ${\cal O}(10^4 {\rm TeV})$, while being consistent with naturalness and perturbativity considerations.
Copyright/License publication: © 2023-2024 The Authors (License: CC-BY-4.0)
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