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CMS-HIG-24-004 ; CERN-EP-2025-173
Model-independent measurement of the Higgs boson associated production with two jets and decaying to a pair of W bosons in proton-proton collisions at $ \sqrt{s} = $ 13 TeV
Submitted to J. High Energy Phys.
Abstract: A model-independent measurement of the differential production cross section of the Higgs boson decaying into a pair of W bosons, with a final state including two jets produced in association, is presented. In the analysis, events are selected in which the decay products of the two W bosons consist of an electron, a muon, and missing transverse momentum. The model independence of the measurement is maximized by making use of a discriminating variable that is agnostic to the signal hypothesis developed through machine learning. The analysis is based on proton-proton collision data at $ \sqrt{s}= $ 13 TeV collected with the CMS detector from 2016-2018, corresponding to an integrated luminosity of 138 fb$^{-1}$. The production cross section is measured as a function of the difference in azimuthal angle between the two jets. The differential cross section measurements are used to constrain Higgs boson couplings within the standard model effective field theory framework.
Figures & Tables Summary References CMS Publications
Figures

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Figure 1:
Normalized VBF differential cross section as a function of the signed azimuthal angle difference between the two jets, with the Higgs boson mass assumed to be 125 GeV. Different hypotheses are superimposed corresponding to a mixed $ CP $ scenario, a pure $ CP $-even AC, a pure $ CP $-odd AC, and an SM coupling in the HVV vertex.

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Figure 2:
Normalized distributions of $ \mathcal{D}_\mathrm{VBF} $ (left) and $ \mathcal{D}_\mathrm{ggH} $ (right), evaluated on signal and background events using the ADNNs trained on even-numbered MC events. The signal predictions are displayed as an envelope representing the range of algorithm outputs across all signal hypotheses included in the training. The background class contributions from SM ggH (left) and SM VBF (right) events are highlighted using dashed lines. For $ \mathcal{D}_\mathrm{VBF} $, the background class contains ggH events according to the SM proportion, and the corresponding contribution is rescaled by a factor of 50 to enhance visibility in the plot; for $ \mathcal{D}_\mathrm{ggH} $, the background class contains 50% VBF events.

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Figure 2-a:
Normalized distributions of $ \mathcal{D}_\mathrm{VBF} $ (left) and $ \mathcal{D}_\mathrm{ggH} $ (right), evaluated on signal and background events using the ADNNs trained on even-numbered MC events. The signal predictions are displayed as an envelope representing the range of algorithm outputs across all signal hypotheses included in the training. The background class contributions from SM ggH (left) and SM VBF (right) events are highlighted using dashed lines. For $ \mathcal{D}_\mathrm{VBF} $, the background class contains ggH events according to the SM proportion, and the corresponding contribution is rescaled by a factor of 50 to enhance visibility in the plot; for $ \mathcal{D}_\mathrm{ggH} $, the background class contains 50% VBF events.

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Figure 2-b:
Normalized distributions of $ \mathcal{D}_\mathrm{VBF} $ (left) and $ \mathcal{D}_\mathrm{ggH} $ (right), evaluated on signal and background events using the ADNNs trained on even-numbered MC events. The signal predictions are displayed as an envelope representing the range of algorithm outputs across all signal hypotheses included in the training. The background class contributions from SM ggH (left) and SM VBF (right) events are highlighted using dashed lines. For $ \mathcal{D}_\mathrm{VBF} $, the background class contains ggH events according to the SM proportion, and the corresponding contribution is rescaled by a factor of 50 to enhance visibility in the plot; for $ \mathcal{D}_\mathrm{ggH} $, the background class contains 50% VBF events.

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Figure 3:
Post-fit $ \mathcal{D}_\mathrm{VBF} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 3. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. A uniform binning is applied for visualization, with the true binning range indicated on the $ x $ axis. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 3-a:
Post-fit $ \mathcal{D}_\mathrm{VBF} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 3. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. A uniform binning is applied for visualization, with the true binning range indicated on the $ x $ axis. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 3-b:
Post-fit $ \mathcal{D}_\mathrm{VBF} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 3. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. A uniform binning is applied for visualization, with the true binning range indicated on the $ x $ axis. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 3-c:
Post-fit $ \mathcal{D}_\mathrm{VBF} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 3. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. A uniform binning is applied for visualization, with the true binning range indicated on the $ x $ axis. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 3-d:
Post-fit $ \mathcal{D}_\mathrm{VBF} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 3. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. A uniform binning is applied for visualization, with the true binning range indicated on the $ x $ axis. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 4:
Post-fit $ \mathcal{D}_\mathrm{VBF,ggH} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 1. The 2D distribution is unrolled into a 1D histogram, where the $ x $-axis labels correspond to the bin numbering of the original 2D map. Dashed black vertical lines mark the boundaries between $ \mathcal{D}_\mathrm{ggH} $ intervals, within which the binning reflects the $ \mathcal{D}_\mathrm{VBF} $ subdivisions. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 4-a:
Post-fit $ \mathcal{D}_\mathrm{VBF,ggH} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 1. The 2D distribution is unrolled into a 1D histogram, where the $ x $-axis labels correspond to the bin numbering of the original 2D map. Dashed black vertical lines mark the boundaries between $ \mathcal{D}_\mathrm{ggH} $ intervals, within which the binning reflects the $ \mathcal{D}_\mathrm{VBF} $ subdivisions. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 4-b:
Post-fit $ \mathcal{D}_\mathrm{VBF,ggH} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 1. The 2D distribution is unrolled into a 1D histogram, where the $ x $-axis labels correspond to the bin numbering of the original 2D map. Dashed black vertical lines mark the boundaries between $ \mathcal{D}_\mathrm{ggH} $ intervals, within which the binning reflects the $ \mathcal{D}_\mathrm{VBF} $ subdivisions. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 4-c:
Post-fit $ \mathcal{D}_\mathrm{VBF,ggH} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 1. The 2D distribution is unrolled into a 1D histogram, where the $ x $-axis labels correspond to the bin numbering of the original 2D map. Dashed black vertical lines mark the boundaries between $ \mathcal{D}_\mathrm{ggH} $ intervals, within which the binning reflects the $ \mathcal{D}_\mathrm{VBF} $ subdivisions. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 4-d:
Post-fit $ \mathcal{D}_\mathrm{VBF,ggH} $ distributions in the $ \Delta\Phi_\mathrm{{jj}} $ bins of the SR for the 2016-2018 data set, corresponding to fit configuration 1. The 2D distribution is unrolled into a 1D histogram, where the $ x $-axis labels correspond to the bin numbering of the original 2D map. Dashed black vertical lines mark the boundaries between $ \mathcal{D}_\mathrm{ggH} $ intervals, within which the binning reflects the $ \mathcal{D}_\mathrm{VBF} $ subdivisions. Systematic uncertainties are shown as dashed gray bands. The pre-fit signal is shown superimposed as a dotted line, while the post-fit signal is included in the stacked histograms on top of the background templates. The binning scheme optimized for the 2018 data set is used. The lower panel shows the ratio of data to the total expected yield, where the signal contribution is included in the expectation.

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Figure 5:
Measured fiducial cross section of the VBF and ggH production processes. Colored markers represent the extracted cross section values from data, with error bars showing the combined statistical and systematic uncertainties: red for VBF, light blue for ggH, and violet for the sum of VBF + ggH. The gray bands indicate the statistical uncertainties. The colored histogram corresponds to the expected SM prediction, simulated with POWHEG + JHUGEN + PYTHIA generators. The lower panel displays the ratio of the measured values to the SM expectation.

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Figure 6:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-a:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-b:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-c:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-d:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-e:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 6-f:
Two-dimensional expected and observed scans for the pairs of Wilson coefficients $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (upper left), $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (upper right), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle left), $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (middle right), $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (lower left) and $ c_{\text{Hj1}} $, $ c_{\text{Hj3}} $ (lower right). Solid (dotted) lines correspond to the 68% (95%) CL contours.

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Figure 7:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-a:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-b:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-c:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-d:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-e:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 7-f:
Expected and observed scans for the Wilson coefficients $ c_\text{HW} $ (upper left), $ c_\text{HWB} $ (middle left), $ c_\text{HB} $ (lower left), $ c_{\text{H}\tilde{\text{W}}} $ (upper right), $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (middle right) and $ c_{\text{H}\tilde{\text{B}}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 8:
Expected and observed scans for the Wilson coefficients $ c_\text{Hu} $ (upper left), $ c_{\text{Hd}} $ (upper right), $ c_{\text{Hj1}} $ (lower left) and $ c_{\text{Hj3}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the other coefficient from the $ (c_\text{Hu},c_{\text{Hd}}) $ and $ (c_\text{Hj1},c_{\text{Hj3}}) $ pairs, respectively, is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 8-a:
Expected and observed scans for the Wilson coefficients $ c_\text{Hu} $ (upper left), $ c_{\text{Hd}} $ (upper right), $ c_{\text{Hj1}} $ (lower left) and $ c_{\text{Hj3}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the other coefficient from the $ (c_\text{Hu},c_{\text{Hd}}) $ and $ (c_\text{Hj1},c_{\text{Hj3}}) $ pairs, respectively, is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 8-b:
Expected and observed scans for the Wilson coefficients $ c_\text{Hu} $ (upper left), $ c_{\text{Hd}} $ (upper right), $ c_{\text{Hj1}} $ (lower left) and $ c_{\text{Hj3}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the other coefficient from the $ (c_\text{Hu},c_{\text{Hd}}) $ and $ (c_\text{Hj1},c_{\text{Hj3}}) $ pairs, respectively, is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 8-c:
Expected and observed scans for the Wilson coefficients $ c_\text{Hu} $ (upper left), $ c_{\text{Hd}} $ (upper right), $ c_{\text{Hj1}} $ (lower left) and $ c_{\text{Hj3}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the other coefficient from the $ (c_\text{Hu},c_{\text{Hd}}) $ and $ (c_\text{Hj1},c_{\text{Hj3}}) $ pairs, respectively, is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 8-d:
Expected and observed scans for the Wilson coefficients $ c_\text{Hu} $ (upper left), $ c_{\text{Hd}} $ (upper right), $ c_{\text{Hj1}} $ (lower left) and $ c_{\text{Hj3}} $ (lower right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the other coefficient from the $ (c_\text{Hu},c_{\text{Hd}}) $ and $ (c_\text{Hj1},c_{\text{Hj3}}) $ pairs, respectively, is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 9:
Expected and observed scans for the Wilson coefficients $ c_\text{HD} $ (left) and $ c_{\text{H}\Box} $ (right). The results are presented for the scenario where all other coefficients are fixed to their SM values. Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 9-a:
Expected and observed scans for the Wilson coefficients $ c_\text{HD} $ (left) and $ c_{\text{H}\Box} $ (right). The results are presented for the scenario where all other coefficients are fixed to their SM values. Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 9-b:
Expected and observed scans for the Wilson coefficients $ c_\text{HD} $ (left) and $ c_{\text{H}\Box} $ (right). The results are presented for the scenario where all other coefficients are fixed to their SM values. Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 10:
Expected and observed scans for the Wilson coefficients $ c_\text{HG} $ (left) and $ c_{\text{H}\tilde{\text{G}}} $ (right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 10-a:
Expected and observed scans for the Wilson coefficients $ c_\text{HG} $ (left) and $ c_{\text{H}\tilde{\text{G}}} $ (right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 10-b:
Expected and observed scans for the Wilson coefficients $ c_\text{HG} $ (left) and $ c_{\text{H}\tilde{\text{G}}} $ (right). The results are presented for two scenarios: one where all other coefficients are fixed to their SM values (grey) and another where the coefficient with opposite $ CP $-parity is allowed to float in the fit (black). Horizontal lines indicate the one-dimensional 68% and 95% CL values.

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Figure 11:
Measured fiducial cross section for VBF production as a function of $ \Delta\Phi_\mathrm{{jj}} $ (black) compared to various predictions. The cross section predictions include: the SM (red), the ones obtained from the best fit of Wilson coefficients of $ c_\text{HW} $, $ c_{\text{H}\tilde{\text{W}}} $ (yellow), $ c_\text{HWB} $, $ c_{\text{H}\tilde{\text{W}}\text{B}} $ (blue) and $ c_\text{HB} $, $ c_{\text{H}\tilde{\text{B}}} $ (green). The difference between the data and the predictions are displayed in the lower panel.

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Figure 12:
Measured fiducial cross section for VBF production as a function of $ \Delta\Phi_\mathrm{{jj}} $ (black) compared to various predictions. The cross section predictions include: the SM (red), the ones obtained from the best fit of Wilson coefficients of $ c_{\text{H}\Box} $ (dark grey) and $ c_\text{HD} $ (light grey). The difference between the data and the predictions are displayed in the lower panel.

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Figure 13:
Measured fiducial cross section for VBF production as a function of $ \Delta\Phi_\mathrm{{jj}} $ (black) compared to various predictions. The cross section predictions include: the SM (red), the ones obtained from the best fit of Wilson coefficients of $ c_{\text{Hu}} $, $ c_{\text{Hd}} $ (light orange) and $ c_\text{Hj1} $, $ c_{\text{Hj3}} $ (dark orange). The difference between the data and the predictions are displayed in the lower panel.

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Figure 14:
Measured fiducial cross section for ggH production as a function of $ \Delta\Phi_\mathrm{{jj}} $ (black) compared to various predictions. The cross section predictions include: the SM (blue) and the ones obtained from the best fit of Wilson coefficients of $ c_\text{HG} $, $ c_{\text{H}\tilde{\text{G}}} $ (magenta). The difference between the data and the predictions are displayed in the bottom panel.
Tables

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Table 1:
Definition of the analysis phase spaces.

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Table 2:
Definition of the $ \Delta\Phi_\mathrm{{jj}} $ bins.

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Table 3:
Definition of the fiducial phase space. Observables are defined using generator-level quantities.

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Table 4:
Set of ADNN input features.

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Table 5:
Contributions of different sources of uncertainty in the differential cross section measurement, expressed as a percentage of the total uncertainty ($ \Delta \sigma_i / \Delta \sigma_{\text{tot}} \times $ 100). For asymmetric errors, the largest of the up and down uncertainties is reported. The systematic component includes all sources except for background normalization, which is part of the statistical component. Results are shown for each of the four $ \Delta\Phi_\mathrm{{jj}} $ bins.

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Table 6:
Measured fiducial cross section summing VBF and ggH production processes, corresponding to fit configuration 1. The total (statistical and systematic) and statistical uncertainties corresponding to the 68% CL are shown. The observed significance with respect to the background-only hypothesis is computed accounting for the total uncertainty.

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Table 7:
Measured fiducial cross section of VBF and ggH production processes, corresponding to fit configuration 2. The measurement is performed through a simultaneous fit, where the contributions from VBF and ggH production are determined independently in each bin. The observed significance with respect to the background-only hypothesis is computed accounting for the total uncertainty. Negative values or lower uncertainty bounds extending below zero are artifacts of the fit and reflect statistical fluctuations in regions with limited sensitivity.

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Table 8:
Measured fiducial cross section of VBF production process while fixing the ggH process to the SM prediction, corresponding to fit configuration 3. The total (statistical and systematic) and statistical uncertainties corresponding to the 68% CL are shown. The observed significance with respect to the background only hypothesis is computed accounting for the total uncertainty. Negative values or lower uncertainty bounds extending below zero are artifacts of the fit and reflect statistical fluctuations in regions with limited sensitivity.

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Table 9:
List of $ X^{2}H^{2} $, $ H^{4}D^{2} $, and $ \psi^{2}H^{2}D $ operators and their corresponding Wilson coefficients.

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Table 10:
Summary of the constraints on Wilson coefficients, including best fit values, 68% and 95% CL intervals. The observed significance with respect to the SM scenario is shown in the last column. The constraints on $ c_{\text{H}\Box} $ and $ c_\text{HD} $ were obtained from individual fits with all other coefficients fixed to their SM values. For the remaining coefficients, results were obtained from fits where the corresponding $ CP $-even or $ CP $-odd partner was allowed to float, while all other coefficients were fixed to their SM values.
Summary
This paper presents a model-independent measurement of the Higgs boson differential production cross section in its decay to a pair of W bosons, with a final state that includes two jets, two different-flavor leptons $ (\mathrm{e}\mu) $, and missing transverse momentum. The model independence of the measurement is maximized by making use of a signal discriminating variable that is agnostic to the signal hypothesis developed through an adversarial deep neural network. The measurement is based on proton-proton collision data recorded with the CMS detector between 2016 and 2018, corresponding to an integrated luminosity of 138 fb$ ^{-1} $ at a center-of-mass energy of 13 TeV. The production cross section is measured as a function of the azimuthal angle difference between the two jets. Three different signal extraction configurations are employed to measure the Higgs boson production cross section in association with two jets via vector boson fusion (VBF) and gluon-gluon fusion (ggH). Differential cross section measurements are further utilized to constrain Wilson coefficients within the standard model effective field theory framework. The most stringent constraints are obtained on the Charge conjugation Parity ($ CP $)-even $ c_\text{HW} $ and $ c_\text{Hj3} $ coefficients from the VBF cross section measurement, and on the $ CP $-even $ c_\text{HG} $ coefficient from the ggH cross section measurement. All results are found to be consistent with the SM expectations.
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