Introduction

Modified Higgs couplings are studied in the κ framework, where modifications of the Higgs-boson couplings are described by coupling strength modifiers at tree level. The coupling to vector bosons is modified by κV (assuming custodial symmetry, κZ = κW), the couplings to fermions by κF or by individual modifiers κt, κb, κc, κτ, κμ, and the loop-induced processes by κg, κγ and κ. In the Standard Model all κi = 1. More details are given in the report by the Higgs boson working group.

Electroweak precision observables (EWPO) constrain the Higgs sector through the virtual contributions of the Higgs boson to the gauge-boson self-energies. At leading-logarithmic accuracy, a universal rescaling of the HVV coupling modifies the oblique parameters S and T, with U = 0. This provides a constraint on κV that is independent of the Higgs signal-strength measurements and does not require any assumption on the total width. Combining the two gives access to the total Higgs-boson width and to decays into final states that are not experimentally accessible.

The effective description is not renormalisable by itself, so a cut-off scale is required. We use Λ = 4πv ≈ 3 TeV as default, the naive-dimensional-analysis estimate of the strong-coupling scale of the electroweak symmetry-breaking sector, and also quote results for Λ = 1 TeV. (This scale is written as Λ with a tilde in the figures; the cut-off of the effective description is Λ* = Λ / |1 - κV2|1/2.)

The EWPO input is described in the SM section. The Higgs signal strengths are taken from the most recent ATLAS and CMS combinations. Full details are given in our latest publication.



Constraints on Higgs couplings

Using the general parametrisation, in which all fermion couplings and loop-induced contributions have independent modifiers, the ATLAS and CMS signal-strength measurements alone give results consistent with the Standard Model. For the HVV modifier the combined fit gives κV = 1.035+0.051-0.053. The largest deviation is found for κ = 1.47+0.25-0.28, corresponding to about 1.7σ.

From the EWPO alone, without any Higgs signal-strength input, we obtain

κV = 1.009+0.012-0.010   for   Λ = 3 TeV
κV = 1.011+0.017-0.013   for   Λ = 1 TeV

This agrees with the determination from the Higgs signal strengths in the resolved parametrisation, κV = 1.005 ± 0.017, but is more precise, owing to the high experimental and theoretical precision of the EWPO, and it does not require the assumption of no invisible or undetected decays.

Constraints on the κi modifiers in the general parametrisation, using Higgs signal-strength measurements from ATLAS (blue), CMS (red) and their combination (green). Since all κi enter quadratically, only their absolute values are constrained. Arrows indicate central values outside the plotting range.
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Constraints in the κVF plane from Higgs signal-strength measurements in the resolved parametrisation (orange), from the EWPO (green), and from their combination (blue). Fits including EWPO use Λ = 3 TeV. The 68% and 95% contours are computed for one degree of freedom in the EWPO-only fit, and for two degrees of freedom otherwise.
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Total width of the Higgs boson

By providing an independent constraint on κV, the EWPO reduce the freedom in the Higgs-coupling fit and allow a determination of the total Higgs-boson width without specifying a particular extension of the Standard Model. The total-width modifier κH2 = ΓH,tot / ΓH,SM is treated as a free parameter of the fit. The results below are for Λ = 3 TeV.

bosonic parametrisation (11 signal strengths + 24 EWPO)ΓH,tot = 4.36+0.63-0.50 MeV
effective parametrisation (31 signal strengths + EWPO)ΓH,tot = 4.08+0.43-0.37 MeV
resolved parametrisation (59 signal strengths + EWPO)ΓH,tot = 3.78+0.30-0.27 MeV

These values are to be compared with the SM prediction ΓH,SM = 4.10 ± 0.06 MeV. Including more signal-strength information tightens the constraint, at the cost of stronger assumptions on the Higgs-boson couplings. The effective and resolved parametrisations determine the total width with a relative precision of about 10% or better.

Reducing Λ from 3 TeV to 1 TeV shifts the central values by -0.04 MeV, independently of the parametrisation, and increases the uncertainties by about 5%, 10% and 15% for the bosonic, effective and resolved parametrisations, respectively.

Scans of Δχ2 versus the total-width modifier κH2 for the different parametrisations. Solid and dashed lines correspond to Λ = 3 TeV and 1 TeV, respectively.
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Invisible and undetected branching fraction

Higgs-boson decays into final states that are not experimentally accessible at the LHC enter the total width through ΓH,tot = ΓH(κ) / (1 - Binv - Bundet), where Binv and Bundet are the invisible and undetected branching fractions. The total-width constraint from the combined EWPO and signal-strength fit therefore translates directly into a constraint on Bi+u = Binv + Bundet. In this formulation Bi+u is determined from the data and does not rely on the SM prediction for the total width, nor on direct searches for invisible Higgs decays.

The limits below are at 95% CL, obtained by integrating the likelihood over the physical region Bi+u > 0, for Λ = 3 TeV. Expected limits are given in parentheses.

bosonic parametrisationBi+u < 0.27   (0.23 expected)
general parametrisationBi+u < 0.17   (0.16 expected)
resolved parametrisationBi+u < 0.09   (0.08 expected)

In the bosonic parametrisation only the HVV coupling is modified, and all other coupling modifiers, most notably the fermionic ones, are set to their SM values. In the general parametrisation Bi+u is fitted together with all κi modifiers, so that no assumption on any coupling modifier is needed. The resolved parametrisation gives the tightest bound, owing to its stronger assumptions on the fermion couplings and the loop-induced processes.

None of these bounds rely on the assumption |κV| ≤ 1, which is commonly used when only signal-strength measurements are available. Imposing that assumption with signal strengths alone gives Bi+u < 0.07 at 95% CL.

Scans of Δχ2 versus Bi+u = Binv + Bundet from the combined fit to EWPO and Higgs signal strengths, for the different parametrisations. Solid and dashed lines correspond to Λ = 3 TeV and 1 TeV, respectively. The signal-strength-only result with |κV| ≤ 1 is shown for comparison.
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Assumptions and caveats

The constraints on κV, ΓH,tot and Bi+u given above rely on a restricted effective interpretation, and the following assumptions should be kept in mind:
  • The EWPO enter only through the leading-logarithmic contribution of a universal HVV rescaling to the oblique parameters S and T, with U = 0.
  • The SM loop structure is otherwise unchanged, custodial symmetry is unbroken, and there are no BSM effects beyond oblique corrections. Modified fermion couplings, vertex corrections and direct loop contributions from new states to the EWPO are not included.
  • A rescaled HVV coupling alone is not a complete renormalisable theory, so the cut-off dependence should be regarded as a leading-logarithmic estimate. A systematic effective-field-theory treatment would require the relevant operators, counterterms and short-distance assumptions.
  • Beyond the one-loop approximation, additional cut-off-sensitive contributions may arise unless they are suppressed or cancelled by the UV completion.
  • The quoted results assume Λ = 3 TeV unless stated otherwise; the dependence on this choice is quantified above.
The bounds therefore apply to this specific effective description rather than to a general BSM scenario.
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