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Research Article

Search for dark matter with the ATLAS detector

ORCID Icon | (Reviewing Editor)
Article: 1058465 | Received 16 Apr 2015, Accepted 01 Jun 2015, Published online: 17 Jul 2015

Figures & data

Figure 1. ATLAS limits on dark matter production with a high transverse momentum photon in the final state, in the framework of the EFT for operators D5 (top left), D8 (top right) and D9 (bottom left). Bottom right: Upper limits on the WIMP–nucleon cross-section in the spin-dependent and spin-independent cases inferred from the high transverse momentum photon results.

Figure 1. ATLAS limits on dark matter production with a high transverse momentum photon in the final state, in the framework of the EFT for operators D5 (top left), D8 (top right) and D9 (bottom left). Bottom right: Upper limits on the WIMP–nucleon cross-section in the spin-dependent and spin-independent cases inferred from the high transverse momentum photon results.

Figure 2. Left: ATLAS limits on the coupling gfgχ in a simplified model where dark matter production at LHC is mediated by a vector boson of mass mV. Right: Upper limits on M when the high transverse momentum photon signal region is used to set limits on an effective theory with a γγχχ vertex.

Figure 2. Left: ATLAS limits on the coupling gfgχ in a simplified model where dark matter production at LHC is mediated by a vector boson of mass mV. Right: Upper limits on M∗ when the high transverse momentum photon signal region is used to set limits on an effective theory with a γγχχ vertex.

Figure 3. Summary of ATLAS upper limits on WIMP–nucleon cross-section for spin-independent (spin-dependent) interactions on the left (right) panel obtained from the mono-W/Z leptonic and hadronic searches.

Figure 3. Summary of ATLAS upper limits on WIMP–nucleon cross-section for spin-independent (spin-dependent) interactions on the left (right) panel obtained from the mono-W/Z leptonic and hadronic searches.

Figure 4. Left: ATLAS upper limits on the visible production cross-section in the resonant production mode for top+dark matter for different values of the resonant effective coupling strength ares. Right: ATLAS upper limits on the visible production cross-section in the non-resonant production mode for top+dark matter, for different values of the non-resonant effective coupling strength anon-res.

Figure 4. Left: ATLAS upper limits on the visible production cross-section in the resonant production mode for top+dark matter for different values of the resonant effective coupling strength ares. Right: ATLAS upper limits on the visible production cross-section in the non-resonant production mode for top+dark matter, for different values of the non-resonant effective coupling strength anon-res.

Figure 5. ATLAS upper limits on the WIMP–nucleon cross-sections in the spin-independent case via the D1 EFT operator (left) and in the spin-dependent case via the D9 EFT operator (right), as function of the WIMP mass mχ.

Figure 5. ATLAS upper limits on the WIMP–nucleon cross-sections in the spin-independent case via the D1 EFT operator (left) and in the spin-dependent case via the D9 EFT operator (right), as function of the WIMP mass mχ.