Heavy ${{\widetilde{\mathit g}}}$ (Gluino) MASS LIMIT INSPIRE search

For ${\mathit m}_{{{\widetilde{\mathit g}}}}$ $>$ 60$-$70 GeV, it is expected that gluinos would undergo a cascade decay via a number of neutralinos and/or charginos rather than undergo a direct decay to photinos as assumed by some papers. Limits obtained when direct decay is assumed are usually higher than limits when cascade decays are included.

Some earlier papers are now obsolete and have been omitted. They were last listed in our PDG 2014 edition: K. Olive, $\mathit et al.$ (Particle Data Group), Chinese Physics C38 070001 (2014) (http://pdg.lbl.gov).

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT
$\bf{ \text{> 700 - 1780}}$ OUR EVALUATION  Range reflects model dependence
$> 1400$ 95 1
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu1A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1650$ 95 1
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu2A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200 GeV
$> 1600$ 95 1
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu3A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1570$ 95 2
AABOUD
2016AC
ATLS ${}\geq{}$2 jets + 1 or 2 ${{\mathit \tau}}$ + $\not E_T$, Tglu1F, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1460$ 95 3
AABOUD
2016J
ATLS 1 ${{\mathit \ell}^{\pm}}$ + ${}\geq{}$4 jets + $\not E_T$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 5 GeV
$> 1650$ 95 4
AABOUD
2016M
ATLS 2 ${{\mathit \gamma}}$ + $\not E_T$, Tglu1D, any NLSP mass
$> 1510$ 95 5
AABOUD
2016N
ATLS ${}\geq{}$4 jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1500$ 95 6
AABOUD
2016N
ATLS ${}\geq{}$4 jets + $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1780$ 95 7
AAD
2016AD
ATLS 0 ${{\mathit \ell}}$ , ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$> 1760$ 95 8
AAD
2016AD
ATLS 1 ${{\mathit \ell}}$ , ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 700 GeV
$> 1300$ 95 9
AAD
2016BB
ATLS 2 same-sign/3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$ 600 GeV
$> 1100$ 95 9
AAD
2016BB
ATLS 2 same-sign/3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$ 300 GeV
$> 1200$ 95 9
AAD
2016BB
ATLS 2 same-sign /3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 600 GeV
$> 1600$ 10
AAD
2016BG
ATLS 1 ${{\mathit \ell}}$ , ${}\geq{}$4 jets, $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$= 100 GeV
$>1400$ 95 11
AAD
2016V
ATLS ${}\geq{}$7 to ${}\geq{}$10 jets + $\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 200 GeV
$>1400$ 95 11
AAD
2016V
ATLS ${}\geq{}$7 to ${}\geq{}$10 jets + $\not E_T$, pMSSM ${{\mathit M}_{{1}}}$ = 60 GeV, ${{\mathit M}_{{2}}}$ = 3 TeV, tan${{\mathit \beta}}$=10, ${{\mathit \mu}}$ $<$ 0
$> 1100$ 95 12
KHACHATRYAN
2016AM
CMS boosted ${{\mathit W}}+{{\mathit b}}$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$80GeV,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$400GeV
$>700$ 95 12
KHACHATRYAN
2016AM
CMS boosted ${{\mathit W}}+{{\mathit b}}$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=0 GeV
$>1050$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$>1300$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu3A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=0
$>1140$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>850$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=20 GeV,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$700 GeV
$>950$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV
$>1100$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu1B,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= 0.5(${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}),{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$400GeV
$> 830$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu1B,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= 0.5(${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}),{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$700GeV
$>1300$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = ${\mathit m}_{{{\mathit t}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1050$ 95 13
KHACHATRYAN
2016BJ
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = ${\mathit m}_{{{\mathit t}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$>1725$ 95 14
KHACHATRYAN
2016BS
CMS jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1750$ 95 14
KHACHATRYAN
2016BS
CMS jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 14
KHACHATRYAN
2016BS
CMS jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1030$ 95 15
KHACHATRYAN
2016BX
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}{{\mathit s}}$ , RPV, ${{\mathit \lambda}_{{332}}^{''}}$ coupling
$> 1280$ 95 16
KHACHATRYAN
2016BY
CMS opposite-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1000 GeV
$> 1030$ 95 16
KHACHATRYAN
2016BY
CMS opposite-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1440$ 95 17
KHACHATRYAN
2016V
CMS jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1600$ 95 17
KHACHATRYAN
2016V
CMS jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 17
KHACHATRYAN
2016V
CMS jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1450$ 95 17
KHACHATRYAN
2016V
CMS jets + $\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>820$ 95 18
AAD
2015BG
ATLS GGM, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$ , tan ${{\mathit \beta}}$ = 30, ${{\mathit \mu}}$ $>$ 600 GeV
$>850$ 95 18
AAD
2015BG
ATLS GGM, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$ , tan ${{\mathit \beta}}$ = 1.5, ${{\mathit \mu}}$ $>$ 450 GeV
$>1150$ 95 19
AAD
2015BV
ATLS general RPC ${{\widetilde{\mathit g}}}$ decays, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$>700$ 95 20
AAD
2015BX
ATLS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit X}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , independent of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$
$>1290$ 95 21
AAD
2015CA
ATLS ${}\geq{}$2 ${{\mathit \gamma}}$ + $\not E_T$, GGM, bino-like NLSP, any NLSP mass
$>1260$ 95 21
AAD
2015CA
ATLS ${}\geq{}$1 ${{\mathit \gamma}}$ + ${{\mathit b}}$-jets + $\not E_T$, GGM, higgsino-bino admix. NLSP and ${{\mathit \mu}}<$0, m(NLSP)$>$450 GeV
$>1140$ 95 21
AAD
2015CA
ATLS ${}\geq{}$1 ${{\mathit \gamma}}$ + jets + $\not E_T$, GGM, higgsino-bino admixture NLSP, all ${{\mathit \mu}}>$0
$> 1225$ 95 22
KHACHATRYAN
2015AF
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1300$ 95 22
KHACHATRYAN
2015AF
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1225$ 95 22
KHACHATRYAN
2015AF
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 22
KHACHATRYAN
2015AF
CMS CMSSM, tan ${{\mathit \beta}}$=30, ${\mathit m}_{{{\widetilde{\mathit g}}}}={\mathit m}_{{{\widetilde{\mathit q}}}}$, $\mathit A_{0}=−$2max(${\mathit m}_{\mathrm {0}},{\mathit m}_{\mathrm {1/2}}$), $\mu >$0
$>1150$ 95 22
KHACHATRYAN
2015AF
CMS CMSSM, tan ${{\mathit \beta}}$=30, $\mathit A_{0}=−$2max(${\mathit m}_{\mathrm {0}},{\mathit m}_{\mathrm {1/2}}$), $\mu >$0
$>1280$ 95 23
KHACHATRYAN
2015I
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1310$ 95 24
KHACHATRYAN
2015X
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1175$ 95 24
KHACHATRYAN
2015X
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1330$ 95 25
AAD
2014AE
ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1700$ 95 25
AAD
2014AE
ATLS jets + $\not E_T$, mSUGRA/CMSSM, ${\mathit m}_{{{\widetilde{\mathit q}}}}$ = ${\mathit m}_{{{\widetilde{\mathit g}}}}$
$> 1090$ 95 26
AAD
2014AG
ATLS ${{\mathit \tau}}$ + jets + $\not E_T$, natural Gauge Mediation
$> 1600$ 95 26
AAD
2014AG
ATLS ${{\mathit \tau}}$ + jets + $\not E_T$, mGMSB, M$_{mess}$ = 250 GeV, ${{\mathit N}_{{5}}}$ = 3, ${{\mathit \mu}}$ $>$ 0, ${{\mathit C}}_{grav}$ = 1
$> 1350$ 95 27
AAD
2014X
ATLS ${}\geq{}4{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\mathit \nu}}$ , $\not\!\!R$
$> 640$ 95 28
AAD
2014X
ATLS ${}\geq{}4{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ , tan $\beta $ = 30, GGM
$> 1000$ 95 29
CHATRCHYAN
2014AH
CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1350$ 95 29
CHATRCHYAN
2014AH
CMS jets + $\not E_T$, CMSSM, ${\mathit m}_{{{\widetilde{\mathit g}}}}$ = ${\mathit m}_{{{\widetilde{\mathit q}}}}$
$> 1000$ 95 30
CHATRCHYAN
2014AH
CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1000$ 95 31
CHATRCHYAN
2014AH
CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1160$ 95 32
CHATRCHYAN
2014I
CMS ets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1130$ 95 32
CHATRCHYAN
2014I
CMS multijets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1210$ 95 32
CHATRCHYAN
2014I
CMS multijets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1260$ 95 33
CHATRCHYAN
2014N
CMS 1${{\mathit \ell}^{\pm}}$+ jets +${}\geq{}2{{\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\mathit \chi}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\mathit \chi}_{{1}}^{0}}}$=0 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}}}>$ ${\mathit m}_{{{\widetilde{\mathit g}}}}$
$> 650$ 95 34
CHATRCHYAN
2014P
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit j}}{{\mathit j}}{{\mathit j}}$ , $\not\!\!R$
$\text{none 200 - 835}$ 95 34
CHATRCHYAN
2014P
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\mathit j}}{{\mathit j}}$ , $\not\!\!R$
35
CHATRCHYAN
2014R
CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $/$ ${{\widetilde{\mathit q}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ simplified model, GMSB, slepton co-NLSP scenario
36
CHATRCHYAN
2014R
CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
• • • We do not use the following data for averages, fits, limits, etc. • • •
$>1600$ 95 37
KHACHATRYAN
2016AY
CMS 1${{\mathit \ell}^{\pm}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 500$ 95 38
KHACHATRYAN
2016BT
CMS 19-parameter pMSSM model, global Bayesian analysis, flat prior
$> 1400$ 95 39
KHACHATRYAN
2016BX
CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit \nu}}$ , RPV, ${{\mathit \lambda}_{{121}}}$ or ${{\mathit \lambda}_{{122}}}{}\not=$0, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}>$ 400 GeV
95 40
AAD
2015AB
ATLS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit S}}}{{\mathit g}}$ , c${{\mathit \tau}}$ = 1 m, ${{\widetilde{\mathit S}}}$ $\rightarrow$ ${{\mathit S}}{{\widetilde{\mathit G}}}$ and ${{\mathit S}}$ $\rightarrow$ ${{\mathit g}}{{\mathit g}}$ , BR = 100$\%$
95 41
AAD
2015AI
ATLS ${{\mathit \ell}^{\pm}}$ + jets + $\not E_T$
$>1600$ 95 19
AAD
2015BV
ATLS pMSSM, M$_{1}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit q}}}}$ $<$ 1500 GeV
$>1280$ 95 19
AAD
2015BV
ATLS mSUGRA, ${\mathit m}_{\mathrm {0}}$ $>$ 2 TeV
$>1100$ 95 19
AAD
2015BV
ATLS via ${{\widetilde{\mathit \tau}}}$, natural GMSB, all ${\mathit m}_{{{\widetilde{\mathit \tau}}}}$
$>1330$ 95 19
AAD
2015BV
ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>1500$ 95 19
AAD
2015BV
ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit q}}}{{\mathit q}}$ , ${{\widetilde{\mathit q}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>1650$ 95 19
AAD
2015BV
ATLS jets + $\not E_T$, ${\mathit m}_{{{\widetilde{\mathit g}}}}$ = ${\mathit m}_{{{\widetilde{\mathit q}}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>850$ 95 19
AAD
2015BV
ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit g}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 550 GeV
$>1270$ 95 19
AAD
2015BV
ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1150$ 95 19
AAD
2015BV
ATLS jets + ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}{{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1320$ 95 19
AAD
2015BV
ATLS jets + ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ decays via sleptons, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1220$ 95 19
AAD
2015BV
ATLS ${{\mathit \tau}}$, ${{\widetilde{\mathit q}}}$ decays via staus, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1310$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$>1220$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\mathit T}_{{1}}}}$ $<$ 1000 GeV
$>1180$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${\mathit m}_{{{\mathit T}_{{1}}}}$ $<$ 1000 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV
$>1260$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit c}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$>880$ 95 19
AAD
2015BV
ATLS jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit s}}{{\mathit b}}$ , RPV, 400 $<$ ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $<$ 1000 GeV
$>1200$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}_{{1}}}{{\mathit b}}$ and ${{\widetilde{\mathit b}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit b}}_{{1}}}}$ $<$ 1000 GeV
$>1250$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$\text{none, 750 - 1250}$ 95 19
AAD
2015BV
ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ decay via offshell ${{\widetilde{\mathit t}}_{{1}}}$ and ${{\widetilde{\mathit b}}_{{1}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 500 GeV
42
AAD
2015CB
ATLS ${{\mathit \ell}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ( ${{\mathit e}}$ $/$ ${{\mathit \mu}}$) ${{\mathit q}}{{\mathit q}}$ , RPV, benchmark gluino, neutralino masses
$>600$ 95 42
AAD
2015CB
ATLS ${{\mathit \ell}}{{\mathit \ell}}$ /${{\mathit Z}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ( ${{\mathit e}}{{\mathit e}}$ $/$ ${{\mathit \mu}}{{\mathit \mu}}$ $/$ ${{\mathit e}}{{\mathit \mu}}$) ${{\mathit q}}{{\mathit q}}$ , RPV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 400 GeV and 0.7 $<$ c$\tau _{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ $3 \times 10^{5}$ mm
$>1100$ 95 42
AAD
2015CB
ATLS jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\widetilde{\mathit G}}}$ , GGM, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 400 GeV and 3 $<$ c$\tau _{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 500 mm
$>1400$ 95 42
AAD
2015CB
ATLS jets or $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , Split SUSY, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV and 15 $<$ c$\tau $ $<$ 300 mm
$>1500$ 95 42
AAD
2015CB
ATLS $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , Split SUSY, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV and 20 $<$ c$\tau $ $<$ 250 mm
$>1000$ 95 43
AAD
2015X
ATLS ${}\geq{}$10 jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\mathit q}}$ (RPV), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=500 GeV
$>917$ 95 43
AAD
2015X
ATLS ${}\geq{}$6,7 jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\mathit q}}$ , (light-quark, $\lambda {}^{''}$ couplings, RPV)
$>929$ 95 43
AAD
2015X
ATLS ${}\geq{}$6,7 jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\mathit q}}$ , (b-quark, $\lambda {}^{''}$ couplings, RPV)
44
KHACHATRYAN
2015AD
CMS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, GMSB, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$
$>1300$ 95 45
KHACHATRYAN
2015AZ
CMS ${}\geq{}$2 ${{\mathit \gamma}}$, ${}\geq{}$1 jet, (Razor), bino-like NLSP, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 375 GeV
$>800$ 95 45
KHACHATRYAN
2015AZ
CMS ${}\geq{}$1 ${{\mathit \gamma}}$, ${}\geq{}$2 jet, wino-like NLSP, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 375 GeV
$> 1280$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, CMSSM
$> 1250$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}_{{1}}}{{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit b}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit b}}_{{1}}}}$ $<$ 900 GeV
$> 1190$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $<$ 1000 GeV
$> 1180$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}=2{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=60 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}<$1000 GeV
$> 1250$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1340$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1300$ 95 46
AAD
2014AX
ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ simplified model, ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit f}}{{\mathit f}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 2 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 300 GeV
$> 950$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
$> 1000$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}_{{1}}}$ with ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $<$ 200 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 118 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV
$> 640$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}_{{1}}}$ with ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit c}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 20 GeV
$> 850$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}_{{1}}}$ with ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\mathit s}}$ simplified model, $\not\!\!R$
$> 860$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 2 ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1040$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit Z}^{(*)}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 520 GeV
$> 1200$ 95 47
AAD
2014E
ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $/$ ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \nu}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$( ${{\mathit \nu}}{{\mathit \nu}}$) ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
$> 1050$ 95 48
CHATRCHYAN
2014H
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, massless ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$> 900$ 95 49
CHATRCHYAN
2014H
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 0.5 ${\mathit m}_{{{\widetilde{\mathit g}}}}$, massless ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$> 1050$ 95 50
CHATRCHYAN
2014H
CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 300 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 900$ 95 51
CHATRCHYAN
2014H
same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}{{\mathit s}}$ simplified model, $\not\!\!R$
1  KHACHATRYAN 2017 searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing four or more jets, no more than one lepton, and missing transverse momentum, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Figs. 16 and 17. Also, assuming gluinos decay only via three-body processes involving third-generation quarks plus a neutralino/chargino, and assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, a branching ratio-independent limit on the gluino mass is given, see Fig. 16.
2  AABOUD 2016AC searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with hadronic jets, 1 or two hadronically decaying ${{\mathit \tau}}$ and $\not E_T$. In Tglu1F, gluino masses are excluded at 95$\%$ C.L. up to 1570 GeV for neutralino masses of 100 GeV or below. Neutralino masses up to 700 GeV are excluded for all gluino masses between 800 GeV and 1500 GeV, while the strongest neutralino-mass exclusion of 750 GeV is achieved for gluino masses around 1400 GeV. See their Fig. 8. Limits are also presented in the context of Gauge-Mediated Symmetry Breaking models: in this case, values of ${{\mathit \Lambda}}$ below 92 TeV are excluded at the 95$\%$ CL, corresponding to gluino masses below 2000 GeV. See their Fig. 9.
3  AABOUD 2016J searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $\not E_T$. Gluino-mediated pair production of stops with a nearly mass-degenerate stop and neutralino are targeted and gluino masses are excluded at 95$\%$ C.L. up to 1460 GeV. A 100$\%$ of stops decaying via charm + neutralino is assumed. The results are also valid in case of 4-body decays ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit f}}{{\mathit f}^{\,'}}{{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ . See their Fig. 8.
4  AABOUD 2016M searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two photons, hadronic jets and $\not E_T$. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95$\%$ C.L. are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like NLSP. See their Fig.$~$3.
5  AABOUD 2016N searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing hadronic jets, large $\not E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1510 GeV are excluded at the 95$\%$ C.L. in a simplified model with only gluinos and the lightest neutralino. See their Fig. 7b.
6  AABOUD 2016N searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing hadronic jets, large $\not E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1500 GeV are excluded at the 95$\%$ C.L. in a simplified model with gluinos decaying via an intermediate ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ to two quarks, a ${{\mathit W}}$ boson and a ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV. See their Fig 8.
7  AAD 2016AD searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing several energetic jets, of which at least three must be identified as ${{\mathit b}}$-jets, large $\not E_T$ and no electrons or muons. No significant excess above the Standard Model expectations is observed. For ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ below 800 GeV, gluino masses below 1780 GeV are excluded at 95$\%$ C.L. for gluinos decaying via bottom squarks. See their Fig. 7a.
8  AAD 2016AD searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of pp collisions at $\sqrt {s }$ = 13 TeV for events containing several energetic jets, of which at least three must be identified as ${{\mathit b}}$-jets, large $\not E_T$ and one electron or muon. Large-radius jets with a high mass are also used to identify highly boosted top quarks. No significant excess above the Standard Model expectations is observed. For ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ below 700 GeV, gluino masses below 1760 GeV are excluded at 95$\%$ C.L. for gluinos decaying via top squarks. See their Fig. 7b.
9  AAD 2016BB searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with exactly two same-sign leptons or at least three leptons, multiple hadronic jets, ${{\mathit b}}$-jets, and $\not E_T$. No significant excess over the Standard Model expectation is found. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in various simplified models (Tglu1D, Tglu1E, Tglu3A). See their Figs. 4.a, 4.b, and 4.d.
10  AAD 2016BG searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $\not E_T$. The data agree with the SM background expectation in the six signal selections defined in the search, and the largest deviation is a 2.1 standard deviation excess. Gluinos are excluded at 95$\%$ C.L. up to 1600 GeV assuming they decay via the lightest chargino to the lightest neutralino as in the model Tglu1B for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=100 GeV, assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}=({\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2. See their Fig.$~$6.
11  AAD 2016V searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with $\not E_T$ various hadronic jet multiplicities from ${}\geq{}$7 to ${}\geq{}$10 and with various ${{\mathit b}}$-jet multiplicity requirements. No significant excess over the Standard Model expectation is found. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in one simplified model (Tglu1E) and a pMSSM-inspired model. See their Fig. 5.
12  KHACHATRYAN 2016AM searched in 19.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with highly boosted ${{\mathit W}}$-bosons and ${{\mathit b}}$-jets, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3C and Tglu3B simplified models, see Fig. 12.
13  KHACHATRYAN 2016BJ searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the following simplified models: Tglu3A and Tglu3D, see Fig. 4, Tglu3B and Tglu3C, see Fig. 5, and Tglu1B, see Fig. 7.
14  KHACHATRYAN 2016BS searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least one energetic jet , no isolated leptons, and significant $\not E_T$, using the transverse mass variable ${{\mathit M}_{{T2}}}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Fig. 10 and Table 3.
15  KHACHATRYAN 2016BX searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing 0 or 1 leptons and ${{\mathit b}}$-tagged jets, coming from R-parity-violating decays of supersymmetric particles. No excess over the expected background is observed. Limits are derived on the gluino mass, assuming the RPV ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}{{\mathit s}}$ decay, see Fig. 7 and 10.
16  KHACHATRYAN 2016BY searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two opposite-sign, same-flavour leptons, jets, and missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4C simplified model, see Fig. 4, and on sbottom masses in the Tsbot3 simplified model, see Fig. 5.
17  KHACHATRYAN 2016V searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least four energetic jets and significant $\not E_T$, no identified isolated electron or muon or charged track. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A, and Tglu3A simplified models, see Fig. 8.
18  AAD 2015BG searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with jets, missing $\mathit E_{T}$, and two opposite-sign same flavor isolated leptons featuring either a kinematic edge, or a peak at the ${{\mathit Z}}$-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds are observed and 95$\%$ C.L. exclusion limits are derived in a GGM simplified model of gluino pair production where the gluino decays into quarks, a ${{\mathit Z}}$-boson, and a massless gravitino LSP, see Fig. 12. Also, limits are set in simplified models with slepton/sneutrino intermediate states, see Fig. 13.
19  AAD 2015BV summarized and extended ATLAS searches for gluinos and first- and second-generation squarks in final states containing jets and missing transverse momentum, with or without leptons or ${\mathit {\mathit b}}$-jets in the $\sqrt {s }$ =8 TeV data set collected in 2012. The paper reports the results of new interpretations and statistical combinations of previously published analyses, as well as new analyses. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in several R-parity conserving models, leading to a generalized constraint on gluino masses exceeding 1150 GeV for lightest supersymmetric particle masses below 100 GeV. See their Figs. 10, 19, 20, 21, 23, 25, 26, 29-37.
20  AAD 2015BX interpreted the results of a wide range of ATLAS direct searches for supersymmetry, during the first run of the LHC using the $\sqrt {s }$ =7 TeV and $\sqrt {s }$ = 8 TeV data set collected in 2012, within the wider framework of the phenomenological MSSM (pMSSM). The integrated luminosity was up to 20.3 ${\mathrm {fb}}{}^{-1}$. From an initial random sampling of 500 million pMSSM points, generated from the 19-parameter pMSSM, a total of 310,327 model points with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ LSP were selected each of which satisfies constraints from previous collider searches, precision measurements, cold dark matter energy density measurements and direct dark matter searches. The impact of the ATLAS Run 1 searches on this space was presented, considering the fraction of model points surviving, after projection into two-dimensional spaces of sparticle masses. Good complementarity is observed between different ATLAS analyses, with almost all showing regions of unique sensitivity. ATLAS searches have good sensitivity at LSP mass below 800 GeV.
21  AAD 2015CA searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with one or more photons, hadronic jets or ${{\mathit b}}$-jets and $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like or higgsino-bino admixtures NLSP, see Fig. 8, 10, 11
22  KHACHATRYAN 2015AF searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least two energetic jets and significant $\not E_T$, using the transverse mass variable ${{\mathit M}_{{T2}}}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(a), or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(b), or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(c). See also Table 5. Exclusions in the CMSSM, assuming tan ${{\mathit \beta}}$ = 30, $\mathit A_{0}$ = $−$2 max(${\mathit m}_{\mathrm {0}}$, ${\mathit m}_{\mathrm {1/2}}$) and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 15.
23  KHACHATRYAN 2015I searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events in which ${\mathit {\mathit b}}$-jets and four ${{\mathit W}}$-bosons are produced. Five individual search channels are combined (fully hadronic, single lepton, same-sign dilepton, opposite-sign dilepton, multilepton). No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 5. Also a simplified model with gluinos decaying into on-shell top squarks is considered, see Fig. 6.
24  KHACHATRYAN 2015X searched in 19.3${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least two energetic jets, at least one of which is required to originate from a ${\mathit {\mathit b}}$ quark, and significant $\not E_T$, using the razor variables ($\mathit M_{R}$) and $\mathit R{}^{2}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ and the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ take place with branching ratios varying between 0, 50 and 100$\%$, see Figs. 13 and 14.
25  AAD 2014AE searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for strongly produced supersymmetric particles in events containing jets and large missing transverse momentum, and no electrons or muons. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos and squarks, see Figures 5, 6 and 7. Limits are also derived in the mSUGRA/CMSSM with parameters tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2$ ${\mathit m}_{\mathrm {0}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 8.
26  AAD 2014AG searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing one hadronically decaying ${{\mathit \tau}}$-lepton, zero or one additional light leptons (electrons or muons), jets and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95$\%$ C.L. are set in several SUSY scenarios. For an interpretation in the minimal GMSB model, see their Fig. 8. For an interpretation in the mSUGRA/CMSSM with parameters tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2$ ${\mathit m}_{\mathrm {0}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 9. For an interpretation in the framework of natural Gauge Mediation, see Fig. 10. For an interpretation in the bRPV scenario, see their Fig. 11.
27  AAD 2014X searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least four leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in an R-parity violating simplified model where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\mathit \nu}}$ , takes place with a branching ratio of 100$\%$, see Fig. 8.
28  AAD 2014X searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least four leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a general gauge-mediation model (GGM) where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ , takes place with a branching ratio of 100$\%$, for two choices of tan $\beta $ = 1.5 and 30, see Fig. 11. Also some constraints on the higgsino mass parameter ${{\mathit \mu}}$ are discussed.
29  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 28. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 26.
30  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a ${{\mathit b}}$-quark. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Figs. 28 and 29. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 26.
31  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a ${{\mathit b}}$-quark. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Figs. 28 and 29. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$0, are also presented, see Fig. 26.
32  CHATRCHYAN 2014I searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing multijets and large $\not E_T$. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos that decay via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ with a 100$\%$ branching ratio, see Fig. 7b, or via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ with a 100$\%$ branching ratio, see Fig. 7c, or via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , see Fig. 7d.
33  CHATRCHYAN 2014N searched in 19.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing a single isolated electron or muon and multiple jets, at least two of which are identified as originating from a ${{\mathit b}}$-quark. No significant excesses over the expected SM backgrounds are observed. The results are interpreted in three simplified models of gluino pair production with subsequent decay into virtual or on-shell top squarks, where each of the top squarks decays in turn into a top quark and a ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, see Fig. 4. The models differ in which masses are allowed to vary.
34  CHATRCHYAN 2014P searched in 19.4 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for three-jet resonances produced in the decay of a gluino in R-parity violating supersymmetric models. No excess over the expected SM background is observed. Assuming a 100$\%$ branching ratio for the gluino decay into three light-flavour jets, limits are set on the cross section of gluino pair production, see Fig. 7, and gluino masses below 650 GeV are excluded at 95$\%$ C.L. Assuming a 100$\%$ branching ratio for the gluino decaying to one b-quark jet and two light-flavour jets, gluino masses between 200 GeV and 835 GeV are excluded at 95$\%$ C L.
35  CHATRCHYAN 2014R searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a slepton co-NLSP simplified model (GMSB) where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ takes place with a branching ratio of 100$\%$, see Fig. 8.
36  CHATRCHYAN 2014R searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 11.
37  KHACHATRYAN 2016AY searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one isolated high transverse momentum lepton (${{\mathit e}}$ or ${{\mathit \mu}}$), hadronic jets of which at least one is identified as coming from a ${{\mathit b}}$-quark, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A simplified model, see Fig. 10, and in the Tglu3B model, see Fig. 11.
38  KHACHATRYAN 2016BT performed a global Bayesian analysis of a wide range of CMS results obtained with data samples corresponding to 5.0 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV and in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The set of searches considered, both individually and in combination, includes those with all-hadronic final states, same-sign and opposite-sign dileptons, and multi-lepton final states. An interpretation was given in a scan of the 19-parameter pMSSM. No scan points with a gluino mass less than 500 GeV survived and 98$\%$ of models with a squark mass less than 300 GeV were excluded.
39  KHACHATRYAN 2016BX searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing 4 leptons coming from R-parity-violating decays of ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit \nu}}$ with ${{\mathit \lambda}_{{121}}}{}\not=$ 0 or ${{\mathit \lambda}_{{122}}}{}\not=$ 0. No excess over the expected background is observed. Limits are derived on the gluino, squark and stop masses, see Fig. 23.
40  AAD 2015AB searched for the decay of neutral, weakly interacting, long-lived particles in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. Signal events require at least two reconstructed vertices possibly originating from long-lived particles decaying to jets in the inner tracking detector and muon spectrometer. No significant excess of events over the expected background was found. Results were interpreted in Stealth SUSY benchmark models where a pair of gluinos decay to long-lived singlinos, ${{\widetilde{\mathit S}}}$, which in turn each decay to a low-mass gravitino and a pair of jets. The 95$\%$ confidence-level limits are set on the cross section ${\times }$ branching ratio for the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit S}}}{{\mathit g}}$ , as a function of the singlino proper lifetime (c${{\mathit \tau}}$). See their Fig. 10(f)
41  AAD 2015AI searched in 20 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing at least one isolated lepton (electron or muon), jets, and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in the CMSSM/mSUGRA, see Fig. 15, in the NUHMG, see Fig. 16, and in various simplified models, see Figs. $18 - 22$.
42  AAD 2015CB searched for events containing at least one long-lived particle that decays at a significant distance from its production point (displaced vertex, DV) into two leptons or into five or more charged particles in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The dilepton signature is characterised by DV formed from at least two lepton candidates. Four different final states were considered for the multitrak signature, in which the DV must be accompanied by a high-transverse momentum muon or electron candidate that originates from the DV, jets or missing transverse momentum. No events were observed in any of the signal regions. Results were interpreted in SUSY scenarios involving $\mathit R$-parity violation, split supersymmetry, and gauge mediation. See their Fig. $12 - 20$.
43  AAD 2015X searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing large number of jets, no requirements on missing transverse momentum and no isolated electrons or muons. The sensitivity of the search is enhanced by considering the number of ${{\mathit b}}$-tagged jets and the scalar sum of masses of large-radius jets in an event. No evidence was found for excesses above the expected level of Standard Model background. Exclusion limits at 95$\%$ C.L. are set on the gluino mass assuming the gluino decays to various quark flavors, and for various neutralino masses. See their Fig. $11 - 16$.
44  KHACHATRYAN 2015AD searched in 19.4 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two opposite-sign same flavor isolated leptons featuring either a kinematic edge, or a peak at the ${{\mathit Z}}$-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds is observed and 95$\%$ C.L. exclusion limits are derived in a simplified model of gluino pair production where the gluino decays into quarks, a ${{\mathit Z}}$-boson, and a massless gravitino LSP, see Fig. 9.
45  KHACHATRYAN 2015AZ searched in 19.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with either at least one photon, hadronic jets and $\not E_T$ (single photon channel) or with at least two photons and at least one jet and using the razor variables. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for both a bino-like and wino-like neutralino NLSP scenario, see Fig. 8 and 9.
46  AAD 2014AX searched in 20.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for the strong production of supersymmetric particles in events containing either zero or at last one high high-$p_T$ lepton, large missing transverse momentum, high jet multiplicity and at least three jets identified as originating from ${{\mathit b}}$-quarks. No excess over the expected SM background is observed. Limits are derived in mSUGRA/CMSSM models with tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2{{\mathit m}_{{0}}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 14. Also, exclusion limits in simplified models containing gluinos and scalar top and bottom quarks are set, see their Figures 12, 13.
47  AAD 2014E searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for strongly produced supersymmetric particles in events containing jets and two same-sign leptons or three leptons. The search also utilises jets originating from ${{\mathit b}}$-quarks, missing transverse momentum and other variables. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos and squarks, see Figures 5 and 6. In the ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit Z}^{(*)}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, the following assumptions have been made: ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 0.5 ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit g}}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 0.5 (${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 520 GeV. In the ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \nu}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ or ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$( ${{\mathit \nu}}{{\mathit \nu}}$) ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, the following assumptions have been made: ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 0.5 (${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit g}}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 660 GeV. Limits are also derived in the mSUGRA/CMSSM, bRPV and GMSB models, see their Fig. 8.
48  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}}{{\mathit t}}$ , ${{\widetilde{\mathit t}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}}{{\mathit b}}$ , ${{\widetilde{\mathit b}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$, see Fig. 5.
49  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ and ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, see Fig. 7.
50  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, for two choices of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ and fixed ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, see Fig. 6.
51  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the R-parity violating decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\mathit b}}{{\mathit s}}$ takes place with a branching ratio of 100$\%$, see Fig. 8.
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AAD 2015X
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AAD 2015BX
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AAD 2015AI
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AAD 2015BG
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KHACHATRYAN 2015AF
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KHACHATRYAN 2015AD
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KHACHATRYAN 2015X
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KHACHATRYAN 2015I
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AAD 2014AE
JHEP 1409 176 Search for squarks and gluinos with the ATLAS Detector in Final States with Jets and Missing Transverse Momentum using $\sqrt {s }$ = 8 TeV Proton-Proton Collision Data
AAD 2014AX
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AAD 2014X
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AAD 2014E
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JHEP 1409 103 Search for Supersymmetry in Events with Large Missing Transverse Momentum, Jets, and at least one tau Lepton in 20 fb${}^{-1}$ of $\sqrt {s }$ = 8 TeV Proton-Proton Collision Data with the ATLAS Detector
CHATRCHYAN 2014AH
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JHEP 1406 055 Search for New Physics in the Multijet and Missing Transverse Momentum Final State in Proton-Proton Collisions at $\sqrt {s }$ = 8 TeV
CHATRCHYAN 2014H
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CHATRCHYAN 2014N
PL B733 328 Search for Supersymmetry in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV in Events with a Single Lepton, Large Jet Multiplicity, and Multiple $\mathit b$ Jets
CHATRCHYAN 2014P
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CHATRCHYAN 2014R
PR D90 032006 Search for Anomalous Production of Events with Three or More Leptons in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
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