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CMS-EXO-16-049 ; CERN-EP-2018-183
Search for dark matter particles produced in association with a top quark pair at $\sqrt{s} = $ 13 TeV
Phys. Rev. Lett. 122 (2019) 011803
Abstract: A search is performed for dark matter particles produced in association with a top quark pair in proton-proton collisions at $\sqrt{s} = $ 13 TeV. The data correspond to an integrated luminosity of 35.9 fb$^{-1}$ recorded by the CMS detector at the LHC. No significant excess over the standard model expectation is observed. The results are interpreted using simplified models of dark matter production via spin-0 mediators that couple to dark matter particles and to standard model quarks, providing constraints on the coupling strength between the mediator and the quarks. These are the most stringent collider limits to date for scalar mediators, and the most stringent for pseudoscalar mediators at low masses.
Figures Summary References CMS Publications
Figures

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Figure 1:
Selected $ {{p_{\mathrm {T}}} ^\text {miss}} $ distributions in SRs: 2RTT SR for the all-hadronic (upper left), the $\ell $+jets (upper right), and the different-flavor, $ {{m_{\mathrm {T2}}} ^{\ell \ell}} > $ 110 GeV SR in the dileptonic channel (lower). The solid red line shows the expectation for a signal with $m_ {\mathrm {a}} = $ 100 GeV and $m_{\chi} = $ 1 GeV. The last bin contains the overflow events. The lower panel shows the ratio of the observed to the fitted distribution (points), and the ratio of the background expectation before the fit to the fitted distribution (dashed magenta line). The vertical bars indicate the statistical uncertainty on the data. The horizontal bars on the rightmost plot indicate the bin width. The uncertainty bands in both panels include the statistical and systematic uncertainties on the total background.

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Figure 1-a:
Selected $ {{p_{\mathrm {T}}} ^\text {miss}} $ distributions in SRs: 2RTT SR for the all-hadronic. The solid red line shows the expectation for a signal with $m_ {\mathrm {a}} = $ 100 GeV and $m_{\chi} = $ 1 GeV. The last bin contains the overflow events. The lower panel shows the ratio of the observed to the fitted distribution (points), and the ratio of the background expectation before the fit to the fitted distribution (dashed magenta line). The vertical bars indicate the statistical uncertainty on the data. The horizontal bars on the rightmost plot indicate the bin width. The uncertainty bands in both panels include the statistical and systematic uncertainties on the total background.

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Figure 1-b:
Selected $ {{p_{\mathrm {T}}} ^\text {miss}} $ distributions in SRs: 2RTT SR for the $\ell $+jets. The solid red line shows the expectation for a signal with $m_ {\mathrm {a}} = $ 100 GeV and $m_{\chi} = $ 1 GeV. The last bin contains the overflow events. The lower panel shows the ratio of the observed to the fitted distribution (points), and the ratio of the background expectation before the fit to the fitted distribution (dashed magenta line). The vertical bars indicate the statistical uncertainty on the data. The horizontal bars on the rightmost plot indicate the bin width. The uncertainty bands in both panels include the statistical and systematic uncertainties on the total background.

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Figure 1-c:
Selected $ {{p_{\mathrm {T}}} ^\text {miss}} $ distributions in SRs: 2RTT SR for the different-flavor, $ {{m_{\mathrm {T2}}} ^{\ell \ell}} > $ 110 GeV SR in the dileptonic channel. The solid red line shows the expectation for a signal with $m_ {\mathrm {a}} = $ 100 GeV and $m_{\chi} = $ 1 GeV. The last bin contains the overflow events. The lower panel shows the ratio of the observed to the fitted distribution (points), and the ratio of the background expectation before the fit to the fitted distribution (dashed magenta line). The vertical bars indicate the statistical uncertainty on the data. The horizontal bars on the rightmost plot indicate the bin width. The uncertainty bands in both panels include the statistical and systematic uncertainties on the total background.

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Figure 2:
The exclusion limits at 95% CL on the signal strength $\mu =\sigma /\sigma _{\text {th}}$ computed as a function of the mediator and dark matter mass, assuming a scalar (left) and pseudoscalar (right) mediator. The mediator couplings are assumed to be $ {{\mathrm {g}} _{{\mathrm {q}}}} = {\mathrm {g}} _{\chi}=$ 1. The dashed magenta lines represent the 68% probability interval around the expected limit. The observed limit contour is almost coincident with the boundary of the 68% probability interval.

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Figure 2-a:
The exclusion limits at 95% CL on the signal strength $\mu =\sigma /\sigma _{\text {th}}$ computed as a function of the mediator and dark matter mass, assuming a scalar mediator. The mediator couplings are assumed to be $ {{\mathrm {g}} _{{\mathrm {q}}}} = {\mathrm {g}} _{\chi}=$ 1. The dashed magenta lines represent the 68% probability interval around the expected limit. The observed limit contour is almost coincident with the boundary of the 68% probability interval.

png pdf
Figure 2-b:
The exclusion limits at 95% CL on the signal strength $\mu =\sigma /\sigma _{\text {th}}$ computed as a function of the mediator and dark matter mass, assuming a pseudoscalar mediator. The mediator couplings are assumed to be $ {{\mathrm {g}} _{{\mathrm {q}}}} = {\mathrm {g}} _{\chi}=$ 1. The dashed magenta lines represent the 68% probability interval around the expected limit. The observed limit contour is almost coincident with the boundary of the 68% probability interval.

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Figure 3:
The 95% observed and median expected CL upper limits on the coupling strength of the mediator to the standard model quarks under the assumption that $ {\mathrm {g}} _{\chi}= $ 1. A dark matter particle with a mass of 1 GeV is assumed. The green and yellow bands indicate respectively the 68% and 95% probability intervals around the expected limit. The interpretations for a scalar (left) and a pseudoscalar (right) mediator are shown.

png pdf
Figure 3-a:
The 95% observed and median expected CL upper limits on the coupling strength of the mediator to the standard model quarks under the assumption that $ {\mathrm {g}} _{\chi}= $ 1. A dark matter particle with a mass of 1 GeV is assumed. The green and yellow bands indicate respectively the 68% and 95% probability intervals around the expected limit. The interpretations for a scalar mediator are shown.

png pdf
Figure 3-b:
The 95% observed and median expected CL upper limits on the coupling strength of the mediator to the standard model quarks under the assumption that $ {\mathrm {g}} _{\chi}= $ 1. A dark matter particle with a mass of 1 GeV is assumed. The green and yellow bands indicate respectively the 68% and 95% probability intervals around the expected limit. The interpretations for a pseudoscalar mediator are shown.
Summary
In summary, a comprehensive search for dark matter particles produced in association with a top quark pair yields no significant excess over the predicted background. The results presented in this Letter provide 30--60% better cross section limits compared to earlier searches targeting the same signature [57,59]. The analysis offers stronger constraints than direct and indirect experiments for dark matter masses of O(10 GeV) and below. Over much of the parameter space, the $\mathrm{ t \bar{t} } + \chi \overline{\chi}$ signature has better sensitivity for spin-0 mediators than dark matter production in association with a jet [14] -- previously considered to be the most sensitive signature. For the pseudoscalar model, the $\mathrm{ t \bar{t} } + \chi \overline{\chi}$ signature provides the most stringent cross section constraints for mediator masses of around 200 GeV and below. The observed (expected) limits exclude a pseudoscalar mediator with mass below 220 (320) GeV under the $\mathrm{g}_{\mathrm{q}}=\mathrm{g}_{\chi}=$ 1 benchmark scenario. The $\mathrm{ t \bar{t} } + \chi \overline{\chi}$ signature provides the best sensitivity for the scalar mediator model and is currently the only collider signature that is sufficiently sensitive to exclude regions of parameter space with these values of the couplings. The observed exclusion of a mediator with mass below 160 GeV (240 GeV expected) provides the most stringent constraint to date on this model.
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