Results of a search for new physics in final states with an energetic jet and large missing transverse momentum are reported. The search uses proton-proton collision data corresponding to an integrated luminosity of 139 fb$^{-1}$ at a center-of-mass energy of 13 TeV collected in the period 2015-2018 with the ATLAS detector at the Large Hadron Collider. Compared to previous publications, in addition to an increase of almost a factor of four in the data size, the analysis implements a number of improvements in the signal selection and the background determination leading to enhanced sensitivity. Events are required to have at least one jet with transverse momentum above 150 GeV and no reconstructed leptons ($e$, $\mu$ or $\tau$) or photons. Several signal regions are considered with increasing requirements on the missing transverse momentum starting at 200 GeV. Overall agreement is observed between the number of events in data and the Standard Model predictions. Model-independent $95%$ confidence-level limits on visible cross sections for new processes are obtained in the range between 736 fb and 0.3 fb. Results are also translated into improved exclusion limits in models with pair-produced weakly interacting dark-matter candidates, large extra spatial dimensions, supersymmetric particles in several compressed scenarios, axion-like particles, and new scalar particles in dark-energy-inspired models. In addition, the data are translated into bounds on the invisible branching ratio of the Higgs boson.
- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Post-fit $p_{\mathrm{T}}^{\mathrm{recoil}}$ distribution:</b> <ul> <li><a href="102093?version=2&table=HistogramCR1mu0b">CR1mu0b</a> <li><a href="102093?version=2&table=HistogramCR1e0b">CR1e0b</a> <li><a href="102093?version=2&table=HistogramCR1L1b">CR1L1b</a> <li><a href="102093?version=2&table=HistogramCR2mu">CR2mu</a> <li><a href="102093?version=2&table=HistogramCR2e">CR2e</a> <li><a href="102093?version=2&table=HistogramSR">SR</a> </ul> <b>Exclusion contours:</b> <ul> <li>Dark Matter axial-vector mediator: <ul> <li><a href="102093?version=2&table=ContourobsDMA">observed</a> <li><a href="102093?version=2&table=Contourobs_p1DMA">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourobs_m1DMA">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=ContourexpDMA">expected</a> <li><a href="102093?version=2&table=Contourexp_p1DMA">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m1DMA">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_p2DMA">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m2DMA">-2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourobs_xsecDMA">observed upper limits on the cross-sections</a> </ul> <li>Dark Matter pseudo-scalar mediator: <ul> <li><a href="102093?version=2&table=ContourobsDMP">observed</a> <li><a href="102093?version=2&table=Contourobs_p1DMP">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourobs_m1DMP">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=ContourexpDMP">expected</a> <li><a href="102093?version=2&table=Contourexp_p1DMP">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m1DMP">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_p2DMP">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m2DMP">-2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourobs_xsecDMP">observed upper limits on the cross-sections</a> </ul> <li>Dark Matter vector mediator: <ul> <li><a href="102093?version=2&table=ContourobsDMV">observed</a> <li><a href="102093?version=2&table=Contourobs_p1DMV">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourobs_m1DMV">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=ContourexpDMV">expected</a> <li><a href="102093?version=2&table=Contourexp_p1DMV">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m1DMV">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_p2DMV">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourexp_m2DMV">-2 $\sigma$ expected</a> </ul> <li>Dark Matter spin-dependent WIMP-nucleon scattering cross-section: <a href="102093?version=2&table=ContourSDneutron">observed</a> <li>Dark Matter spin-independent WIMP-nucleon scattering cross-section: <a href="102093?version=2&table=ContourSInucleon">observed</a> <li>Dark Matter WIMP annihilation rate: <a href="102093?version=2&table=ContourID">observed</a> <li>SUSY stop pair production: <ul> <li><a href="102093?version=2&table=Contourg_obsTT_directCC">observed</a> <li><a href="102093?version=2&table=Contourg_obs_p1TT_directCC">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_obs_m1TT_directCC">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_expTT_directCC">expected</a> <li><a href="102093?version=2&table=Contourg_exp_p1TT_directCC">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m1TT_directCC">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_p2TT_directCC">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m2TT_directCC">-2 $\sigma$ expected</a> </ul> <li>SUSY stop pair production (4-body decay): <ul> <li><a href="102093?version=2&table=Contourg_obsTT_bffN">observed</a> <li><a href="102093?version=2&table=Contourg_obs_p1TT_bffN">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_obs_m1TT_bffN">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_expTT_bffN">expected</a> <li><a href="102093?version=2&table=Contourg_exp_p1TT_bffN">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m1TT_bffN">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_p2TT_bffN">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m2TT_bffN">-2 $\sigma$ expected</a> </ul> <li>SUSY sbottom pair production: <ul> <li><a href="102093?version=2&table=Contourg_obsBB">observed</a> <li><a href="102093?version=2&table=Contourg_obs_p1BB">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_obs_m1BB">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_expBB">expected</a> <li><a href="102093?version=2&table=Contourg_exp_p1BB">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m1BB">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_p2BB">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m2BB">-2 $\sigma$ expected</a> </ul> <li>SUSY squark pair production: <ul> <li><a href="102093?version=2&table=Contourg_obsSS">observed</a> <li><a href="102093?version=2&table=Contourg_obs_p1SS">+1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_obs_m1SS">-1 $\sigma_{\mathrm{theory}}^{\mathrm{PDF+scale}}$ observed</a> <li><a href="102093?version=2&table=Contourg_expSS">expected</a> <li><a href="102093?version=2&table=Contourg_exp_p1SS">+1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m1SS">-1 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_p2SS">+2 $\sigma$ expected</a> <li><a href="102093?version=2&table=Contourg_exp_m2SS">-2 $\sigma$ expected</a> </ul> <li>Dark energy: <a href="102093?version=2&table=ContourDE">observed and expected</a> <li>ADD: <a href="102093?version=2&table=ContourADD">observed and expected</a> <li>Axion-like particles: <a href="102093?version=2&table=ContourALPs">observed and expected</a> </ul> <b>Impact of systematic uncertainties:</b> <a href="102093?version=2&table=Tablesystimpacts">Table</a><br/><br/> <b>Yields of exclusive regions:</b> <a href="102093?version=2&table=TableyieldsEM0">EM0</a> <a href="102093?version=2&table=TableyieldsEM1">EM1</a> <a href="102093?version=2&table=TableyieldsEM2">EM2</a> <a href="102093?version=2&table=TableyieldsEM3">EM3</a> <a href="102093?version=2&table=TableyieldsEM4">EM4</a> <a href="102093?version=2&table=TableyieldsEM5">EM5</a> <a href="102093?version=2&table=TableyieldsEM6">EM6</a> <a href="102093?version=2&table=TableyieldsEM7">EM7</a> <a href="102093?version=2&table=TableyieldsEM8">EM8</a> <a href="102093?version=2&table=TableyieldsEM9">EM9</a> <a href="102093?version=2&table=TableyieldsEM10">EM10</a> <a href="102093?version=2&table=TableyieldsEM11">EM11</a> <a href="102093?version=2&table=TableyieldsEM12">EM12</a><br/><br/> <b>Yields of inclusive regions:</b> <a href="102093?version=2&table=TableyieldsIM0">IM0</a> <a href="102093?version=2&table=TableyieldsIM1">IM1</a> <a href="102093?version=2&table=TableyieldsIM2">IM2</a> <a href="102093?version=2&table=TableyieldsIM3">IM3</a> <a href="102093?version=2&table=TableyieldsIM4">IM4</a> <a href="102093?version=2&table=TableyieldsIM5">IM5</a> <a href="102093?version=2&table=TableyieldsIM6">IM6</a> <a href="102093?version=2&table=TableyieldsIM7">IM7</a> <a href="102093?version=2&table=TableyieldsIM8">IM8</a> <a href="102093?version=2&table=TableyieldsIM9">IM9</a> <a href="102093?version=2&table=TableyieldsIM10">IM10</a> <a href="102093?version=2&table=TableyieldsIM11">IM11</a> <a href="102093?version=2&table=TableyieldsIM12">IM12</a><br/><br/> <b>Cutflows:</b><br/><br/> Signals filtered with a truth $E_\mathrm{T}^\mathrm{miss}$ cut at: <ul> <li> <a href="102093?version=2&table=Tablecutflows150GeV">150 GeV</a> <li> <a href="102093?version=2&table=Tablecutflows350GeV">350 GeV</a> </ul>
The measured $p_{\mathrm{T}}^{\mathrm{recoil}}$ distributions in the $W \rightarrow \mu \nu $ control region, compared with the background predictions as estimated after the simultaneous, binned background-only fit to the data in the control regions. The last bin of the distribution contains overflows.
The measured $p_{\mathrm{T}}^{\mathrm{recoil}}$ distributions in the $W \rightarrow e \nu$ control region, compared with the background predictions as estimated after the simultaneous, binned background-only fit to the data in the control regions. The last bin of the distribution contains overflows.