TY - JOUR
T1 - Searching for heavy leptophilic Z′
T2 - from lepton colliders to gravitational waves
AU - Dasgupta, Arnab
AU - Dev, P. S.Bhupal
AU - Han, Tao
AU - Padhan, Rojalin
AU - Wang, Si
AU - Xie, Keping
N1 - Publisher Copyright:
© The Author(s) 2023.
PY - 2023/12
Y1 - 2023/12
N2 - We study the phenomenology of leptophilic Z′ gauge bosons at the future high-energy e+e− and μ+μ− 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 O(100 GeV), thus providing a unique opportunity for future lepton colliders. Taking U1Lα−Lβ (α, β = e, μ, τ) models as concrete examples, we show that future e+e− and μ+μ− 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 O(104 TeV), while being consistent with naturalness and perturbativity considerations.
AB - We study the phenomenology of leptophilic Z′ gauge bosons at the future high-energy e+e− and μ+μ− 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 O(100 GeV), thus providing a unique opportunity for future lepton colliders. Taking U1Lα−Lβ (α, β = e, μ, τ) models as concrete examples, we show that future e+e− and μ+μ− 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 O(104 TeV), while being consistent with naturalness and perturbativity considerations.
KW - New Gauge Interactions
KW - Phase Transitions in the Early Universe
UR - http://www.scopus.com/inward/record.url?scp=85182863031&partnerID=8YFLogxK
U2 - 10.1007/JHEP12(2023)011
DO - 10.1007/JHEP12(2023)011
M3 - Article
AN - SCOPUS:85182863031
SN - 1126-6708
VL - 2023
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
IS - 12
M1 - 11
ER -