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CMS-SUS-17-011 ; CERN-EP-2019-040
Search for supersymmetry in final states with photons and missing transverse momentum in proton-proton collisions at 13 TeV
JHEP 06 (2019) 143
Abstract: Results are reported for a search for supersymmetry in final states with photons and missing transverse momentum in proton-proton collisions at the LHC. The data sample corresponds to an integrated luminosity of 35.9 fb$^{-1}$ collected at a center-of-mass energy of 13 TeV using the CMS detector. The results are interpreted in the context of models of gauge-mediated supersymmetry breaking. Production cross section limits are set on gluino and squark pair production in this framework. Gluino masses below 1.86 TeV and squark masses below 1.59 TeV are excluded at 95% confidence level.
Figures & Tables Summary References CMS Publications
Figures

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Figure 1:
Diagrams showing the production of signal events in the collision of two protons (p). In gluino (${\mathrm {\tilde{g}}}$) pair production in the T5gg simplified model (left), the gluino decays to a quark-antiquark pair (${\mathrm {q}} {\overline {\mathrm {q}}}$) and a neutralino (${\tilde{\chi}^{0}_{1}}$). In squark (${\mathrm {\tilde{q}}}$) pair production in the T6gg simplified model (right), the squark decays to a quark and a neutralino. In both cases, the neutralino subsequently decays to a photon (${\gamma}$) and a gravitino (${\mathrm{\tilde{G}}}$).

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Figure 1-a:
Diagram showing the gluino (${\mathrm {\tilde{g}}}$) pair production in the collision of two protons (p), in the T5gg simplified model. The gluino decays to a quark-antiquark pair (${\mathrm {q}} {\overline {\mathrm {q}}}$) and a neutralino (${\tilde{\chi}^{0}_{1}}$). The neutralino subsequently decays to a photon (${\gamma}$) and a gravitino (${\mathrm{\tilde{G}}}$).

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Figure 1-b:
Diagram showing the squark (${\mathrm {\tilde{q}}}$) pair production in the collision of two protons (p), in the T6gg simplified model. The squark decays to a quark and a neutralino. The neutralino subsequently decays to a photon (${\gamma}$) and a gravitino (${\mathrm{\tilde{G}}}$).

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Figure 2:
The top panel shows the observed ${{p_{\mathrm {T}}} ^\text {miss}}$ distribution in data (black points) and predicted background distributions prior to the fit. The vertical line marks the boundary between the validation region ($ {{p_{\mathrm {T}}} ^\text {miss}} < $ 100 GeV) and the signal region ($ {{p_{\mathrm {T}}} ^\text {miss}} > $ 100 GeV). The last bin includes all events with $ {{p_{\mathrm {T}}} ^\text {miss}} > $ 250 GeV. The QCD background is shown in red, the EWK background is shown in blue, and the $ {\mathrm {Z}} {\gamma} {\gamma}$ background is shown in green. The ${{p_{\mathrm {T}}} ^\text {miss}}$ distribution shown in pink (purple) corresponds to the T5gg simplified model with $m_{{\mathrm {\tilde{g}}}}= $ 1700 (2000) GeV and $m_{{\tilde{\chi}^{0}_{1}}} = $ 1000 GeV. The bottom panel shows the ratio of observed events to the expected background. The error bars on the ratio correspond to the statistical uncertainty in the number of observed events. The shaded region corresponds to the total uncertainty in the background estimate.

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Figure 3:
The 95% confidence level upper limits on the gluino (left) and squark (right) pair production cross sections as a function of gluino or squark and neutralino masses. The contours show the observed and expected exclusions assuming the NLO+NLL cross sections, with their one standard deviation uncertainties.

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Figure 3-a:
The 95% confidence level upper limits on the gluino pair production cross sections as a function of gluino and neutralino masses. The contours show the observed and expected exclusions assuming the NLO+NLL cross sections, with their one standard deviation uncertainties.

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Figure 3-b:
The 95% confidence level upper limits on the squark pair production cross sections as a function of squark and neutralino masses. The contours show the observed and expected exclusions assuming the NLO+NLL cross sections, with their one standard deviation uncertainties.
Tables

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Table 1:
Event yield and statistical and systematic uncertainties (in numbers of events) in the QCD background estimation for each signal ${{p_{\mathrm {T}}} ^\text {miss}}$ bin.

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Table 2:
Number of expected background and observed data events in the signal region prior to the fit defined in the text. The uncertainty in each expected background yield includes the statistical uncertainty and all of the systematic uncertainties described in Section 5 added in quadrature.
Summary
The results of a search for general gauge-mediated supersymmetry breaking in proton-proton collisions with two photons and missing transverse momentum in the final state are reported. The analysis was performed using data corresponding to 35.9 fb$^{-1}$ of integrated luminosity, recorded with the CMS detector in 2016 at a proton-proton center-of-mass energy of 13 TeV. An excess of events corresponding to 2.4 standard deviations is observed. Limits are determined on the masses of supersymmetric particles in two simplified models using data-driven background estimation methods and NLO+NLL signal cross section calculations.

In both models, the next-to-lightest supersymmetric particle is the neutralino, which decays with a 100% branching fraction to a photon and a gravitino, the lightest supersymmetric particle. The first simplified model assumes gluino pair production, with each gluino decaying to a neutralino and quarks. The second simplified model assumes squark pair production, with each squark decaying to a quark and a neutralino. The expected limits on gluino and squark masses, for the respective models, are 2.02 and 1.74 TeV at 95% confidence level. This is an increase in sensitivity of more than 300 GeV for each model with respect to the analysis performed with 2.3 fb$^{-1}$ of integrated luminosity collected using the CMS detector in 2015. The observed exclusions are for gluino masses less than 1.86 TeV and squark masses less than 1.59 TeV, where the difference between the expected and observed exclusions is driven by the excess observed in the data. The analysis described in this paper improves the observed limits by 210 GeV for gluino masses and 220 GeV for squark masses with respect to the previous CMS result.
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