
This situation motivates the effective field theory (EFT) approach to describe the NP
effects. The Standard Model Effective Field Theory (SMEFT) [12–15] is one of the actively
studied EFTs, and information about the NP effects is transferred to higher-dimensional
operators of EFTs consisting of the SM fields. To generate the SFO-EWPT, a consider-
able amount of literature [16–46] has considered the SMEFT dimension-six ϕ6operator#1.
In the context of the electroweak baryogenesis scenario, the other SMEFT dimension-six
operators [18,25,44–46,48] are also studied. On the experimental grounds, there is grow-
ing interest in the constraints on the SMEFT Wilson coefficients from the current and
past experimental data, and future collider experiments, e.g., high-luminosity LHC [49],
the International Linear Collider (ILC) [50], the Compact LInear Collider (CLIC) [51],
the Future Circular Collider of electrons and positrons (FCC-ee) [52], and the Circular
Electron Positron Collider (CEPC) [53]. Furthermore, the SFO-EWPT predicts stochas-
tic background of gravitational waves (GWs), and its spectrum can be peaked around
the future interferometer experiment band with milli- to deci-Hertz, such as Laser In-
terferometer Space Antenna (LISA) [54], DECi-hertz Interferometer Gravitational wave
Observatory (DECIGO) [55], and Big-Bang Observer (BBO) [56]. Therefore, the sen-
sitivities of future GW observations to the SMEFT ϕ6operator also have been investi-
gated [19,20,27,28,31–33,37,39–41,43,46].
The previous works mainly studied a parameter space to generate a detectable amount
of GWs, but they have not quantified how precisely the NP effects can be measured once
the GWs are detected. In light of these circumstances, in the previous works of the NP
search by the GW observations [57], the method of Fisher matrix analysis was proposed to
evaluate the expected sensitivities to NP model parameters. This analysis quantifies how
precisely the NP model parameters can be measured by the GWs observations, and it is
clarified that the GW observations potentially have higher sensitivities to small deviations
of the Higgs potential by the NP effects than the future collider experiments such as the
ILC-250. This result naturally leads us to study the sub-dominant SMEFT effects on the
Higgs potential and the sensitivities of the GW observations to them.
In this paper, we study the SMEFT dimension-six operator corrections to the Higgs
potential and the sensitivities of the GW observations to them. We will focus on three
types of the SMEFT dimension-six operator effects: (i) SMEFT tree level effect on ϕ6,
(ii) SMEFT tree level effects on the wave function renormalization of the Higgs field, and
(iii) SMEFT one-loop top-quark effects. Type (i) dominates the SMEFT effect on the
Higgs potential and can achieve the SFO-EWPT. Type (ii) is the tree level effects, but
not dominant effects because of the suppression by interference effects with the Higgs self
couplings. Type (iii) arises from the loop diagrams and can not dominate the SMEFT effect,
but it can be a measurable effect because of the large top Yukawa coupling. Therefore, we
focus on a scenario where the SFO-EWPT mainly arises by (i), and the Higgs potential is
#1In Refs. [23,47], the validity of the SMEFT description for the SFO-EWPT is questioned; see Sec. 6.
2