Abstract (data abstract)

Results showing the search for direct production of charginos and neutralinos via electroweak interactions.The results are based on data from proton-proton collisions at a center-of-mass energy of $13~\mathrm{TeV}$ collected with the CMS detector at the LHC, corresponding to an integrated luminosity of $137~\mathrm{fb}^{-1}$.The search considers final states with large missing transverse momentum and pairs of hadronically decaying bosons WW, WZ, and WH, where H is the Higgs boson.These bosons are identified using novel algorithms.No significant excess of events is observed relative to the expectations from the standard model.Limits at the 95\% confidence level are placed on the cross section for production of mass-degenerate wino-like supersymmetric particles $\widetilde{\chi}_{1}^{\pm}$ and $\widetilde{\chi}_{2}^{0}$, and mass-degenerate higgsino-like supersymmetric particles $\widetilde{\chi}_{1}^{\pm}$, $\widetilde{\chi}_{2}^{0}$, and $\widetilde{\chi}_{3}^{0}$.In the limit of a nearly-massless lightest supersymmetric particle $\widetilde{\chi}_{1}^{0}$, wino-like particles with masses up to 870 and $960~\mathrm{GeV}$ are excluded in the cases of $\widetilde{\chi}_{2}^{0}\to\mathrm{Z}\widetilde{\chi}_{1}^{0}$ and $\widetilde{\chi}_{2}^{0}\to\mathrm{H}\widetilde{\chi}_{1}^{0}$, respectively, and higgsino-like particles are excluded between 300 and $650~\mathrm{GeV}$.

Figure 3a

Data from Figure 3 (upper left), located on page 13.

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SM background prediction vs. observation in the b-veto signal region
Figure 3a ratios

Data from Figure 3 (upper left), located on page 13.

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SM background observation/prediction in the bVeto signal region
Figure 3b

Data from Figure 3 (upper right), located on page 13.

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SM background prediction vs. observation in the WH signal region
Figure 3b ratios

Data from Figure 3 (upper right), located on page 13.

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SM background observation/prediction in the WH signal region
Figure 3c

Data from Figure 3 (lower left), located on page 13.

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SM background prediction vs. observation in the W signal region
Figure 3c ratios

Data from Figure 3 (lower left), located on page 13.

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SM background observation/prediction in the W signal region
Figure 3d

Data from Figure 3 (lower right), located on page 13.

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SM background prediction vs. observation in the H signal region
Figure 3d ratios

Data from Figure 3 (lower right), located on page 13.

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SM background observation/prediction in the H signal region
Figure 4a Observed Lines

Data from Figure 4 (upper left), located on page 14.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4a Expected Lines

Data from Figure 4 (upper left), located on page 14.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4a Observed

Data from Figure 4 (upper left), located on page 14.

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The 95% CL observed upper limits on the production cross sections for $\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^\mp_1$ assuming that each $\widetilde{\chi}^\pm_1$ decays to...
Figure 4b Observed Lines

Data from Figure 4 (upper right), located on page 14.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4b Expected Lines

Data from Figure 4 (upper right), located on page 14.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4b Observed

Data from Figure 4 (upper right), located on page 14.

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The 95% CL observed upper limits on the production cross sections for $\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^0_2$ assuming that each $\widetilde{\chi}^\pm_1$ decays to...
Figure 4c Observed Lines

Data from Figure 4 (lower), located on page 14.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4c Expected Lines

Data from Figure 4 (lower), located on page 14.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 4c Observed

Data from Figure 4 (lower), located on page 14.

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The 95% CL observed upper limits on the production cross sections for $\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^0_2$ assuming that each $\widetilde{\chi}^\pm_1$ decays to...
Figure 5a WW WZ Observed Lines

Data from Figure 5 (left), located on page 14.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5a WW WZ Expected Lines

Data from Figure 5 (left), located on page 14.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5a WW WH Observed Lines

Data from Figure 5 (left), located on page 15.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5a WW WH Expected Lines

Data from Figure 5 (left), located on page 15.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5b Observed Lines

Data from Figure 5 (right), located on page 15.

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Observed exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5b Expected Lines

Data from Figure 5 (right), located on page 15.

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Expected exclusion limits assuming the approximate-NLO+NLL cross sections
Figure 5b Observed

Data from Figure 5 (right), located on page 15.

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The 95% CL observed upper limits on the production cross sections for mass-degenerate higgsino-like$\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^\mp_1$, $\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^0_2$, $\widetilde{\chi}^\pm_1$ $\widetilde{\chi}^0_3$ and...

Figure 3a

Figure 3a ratios

Figure 3b

Figure 3b ratios

Figure 3c

Figure 3c ratios

Figure 3d

Figure 3d ratios

Figure 4a Observed Lines

Figure 4a Expected Lines

Figure 4a Observed

Figure 4b Observed Lines

Figure 4b Expected Lines

Figure 4b Observed

Figure 4c Observed Lines

Figure 4c Expected Lines

Figure 4c Observed

Figure 5a WW WZ Observed Lines

Figure 5a WW WZ Expected Lines

Figure 5a WW WH Observed Lines

Figure 5a WW WH Expected Lines

Figure 5b Observed Lines

Figure 5b Expected Lines

Figure 5b Observed

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