PoS(EPS-HEP 2013)161 http://pos.sissa.it/ ∗ oliver.buchmueller@cern.ch Speaker. Since its first physics operation inin 2010, searches the for Large Hadron supersymmetry. Collider This atstatus proceeding CERN of report has searches provides set for a a supersymmetry brief precedent at overview the on LHC. the current ∗ Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. c

The European Physical Society Conference on18-24 High July Energy 2013 Physics -EPS-HEP2013 Stockholm, Sweden on behalf of the ATLAS and CMS Collaborations Oliver Buchmueller Searches for Supersymmetry Imperial College London E-mail: PoS(EPS-HEP 2013)161 are L and [GeV] 0 B 3 b-jets m Oliver Buchmueller , where S 2 not included. )+ L SUSY theory ATLAS-CONF-2013-047 arXiv: 1308.1841 ATLAS-CONF-2013-061 ATLAS-CONF-2013-062 ATLAS-CONF-2013-026 ATLAS-CONF-2013-007 0-lepton, 2-6 jets 0-lepton, 7-10 jets 0-1 lepton, 3 b-jets 1-lepton + jets + MET 1-2 taus + jets + MET 2-SS-leptons, 0 - − B

(1400 GeV) (

~ g 3 ) of integrated luminosity each at 1 1 − − Expected Observed Expected Observed Expected Observed Expected Observed Expected Observed Expected Observed = ( 95% CL limits. limits. CL 95% R

h (126 GeV) of data at this energy. 1 − > 0 µ = 8 TeV 8 = 2 , s 0 , -1 ~q (2000 GeV) = -2m 0 ]. For more details on LEP and Tevatron results see also Preliminary 3 ] had collected about 5 fb 2

h (124 GeV) is the spin, is conserved the lightest SUSY particle (LSP) is ) = 30, A ) = 30, S ~q (1600 GeV) L dt = 20.1 - 20.7 fb 20.7 - 20.1 = dt L ATLAS

(1000 GeV)

h (122 GeV) ~ g ]. 95% C.L. limits for different ATLAS searches defined in the CMSSM 4 ] and ATLAS [ 1 LSP MSUGRA/CMSSM: MSUGRA/CMSSM: tan( 2013 SUSY Status: 0 1000 2000 3000 4000 5000 6000 Figure 1: 300 600 500 400 700 900 800

1000

1/2 [GeV] m If the multiplicative quantum number of R-parity, The landscape of searches for Supersymmetry (SUSY) has changed dramatically since the In this proceeding report I will focus on the status of searches for SUSY at the LHC. A more 2. Summary of R-parity conserving searches earlier PDG reviews [ stable and often assumed to bethrough a the weakly experiment, interacting leading massive particle. toenergy, final The and states LSP possible escapes with leptons undetected several and hadronic photons jets, in the large final missing state. transverse 1. Introduction Large Hadron Collider (LHC) atexperiments CERN CMS began [ physics operation in 2010. By the end of 2011 the a center-of-mass energy of 7 TeV.and In each 2012 experiment the collected LHC approximately operated 20 at fb a center-of-mass energy of 8 TeV baryon and lepton numbers and detailed and comprehensive overview is provided in thereview September for 2013 SUSY update of searches the in experimental the PDG [ Searches for Supersymmetry ! !

PoS(EPS-HEP 2013)161 , 0 m 2 , lim- − 2 ! ]! = 37 0 SUSY A ˜ g GeV m [ m 1500! 30, 0 1 0 1 0 1 = BR=100%! alllimits are ! observednominal ! 95%CLs limits ! conserved ! RP Oliver Buchmueller ¯ t = ¯ b ¯ q t mediated! b q β ! ! ! SUSY ˜ g ˜ g ˜ ! ! ATLAS-CONF-2013-061 g ! ! ATLAS-CONF-2013-047 ! ! CMS-PAS-SUS-12-024 m Gluino 1250! ) l ˜ ) 0 2 l ˜

shows an illustrative overview of t m 2 2 0 heavy

= (

light 0 2

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± 1

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± 1

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! ! 2 m =

< CMS-PAS

SUSY SUSY

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3

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!

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m LSP

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!

m

= t ˜

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! CMS-PAS-SUS-12-028 ! CMS-PAS-SUS ! -13-011

! CMS-PAS-SUS-12-028 ! ATLAS-CONF-2013-053 ! ATLAS-CONF-2013-037 0 1 m 0 1 SUSY 0 1 0 1 0 1 0 1 slepton 0 1 ! ATLAS-CONF-2013-068 250! m Direct q 0 1 u t b SUSY ± ± l l c Wb m ! ! ! ! Illustrative summary plot for the most important simplified model limits. ! ˜ ! q b Direct ˜ t ˜ L ! ! “gap” Directin stop ! ˜ R u L shows limits in the framework of the CMSSM, assuming tan ˜ t ! ATLAS-CONF- 2013-049! ˜ t l ˜ l ˜ 1 0! ]! ! 0! Figure 2: LSP

GeV 500! 1000!

250! 750! 0, for several ATLAS searches. In this constrained SUSY model gluino masses below [ m

EPS 2013 Direct SUSY Searches, O. O. Searches, SUSY Direct 2013 EPS

Buchmüller > For gluino masses rather similar limits, ranging from 1.2 TeV to 1.4 TeV, are obtainedLimits from defined in simplified models on squark mass are not only much weaker but also vary Another important interpretation approach, even less dependent on fundamental assumptions, ATLAS and CMS have performed many searches looking for R-parity conserving SUSY sig- µ 1.3 TeV are excluded for all squark masses, while for equal gluino and squark masses, the limit is its on direct squark production only go up 800 GeV under the assumption of an eightfold mass- different model assumptions. This shows that thespace LHC for is probing direct a gluino large production region at in SUSY the parameter 1 TeV scale and beyond. strongly depending on the assumed properties of the decay chain. As shown in Figure limits for the most important simplified models that are considered. is the characterisation of the searchesset in of terms SUSY of particle simplified production models. and Such decayother models modes parameters and assume leave freely. a open limited Today, the ATLAS possibility andframework to CMS vary to masses have provide and adopted interpretations simplified of models their as searches. the Figure primary natures. Figure and ≈ around 1.7 TeV. Furthermore, squark masses below 1.6CMS TeV are collaboration excluded for has all not gluino masses. yetbut The provided the an performance interpretation is of expected to their be 8 very TeV similar. searches in the CMSSM Searches for Supersymmetry PoS(EPS-HEP 2013)161 ] 5 are i jk 1800 = 7 TeV = 8 TeV s s 1600 Oliver Buchmueller Mass scales [GeV] EPSHEP 2013 EPSHEP CMS Preliminary Prompt LSP decays 1400 1200 1000 appear in the super potential, where 00 i jk λ 4 800 and 0 i jk λ , 600 i jk λ 450 GeV for the best possible scenario of very light neutrali- ≈ 400 200 EXO-12-049 L=19.5 /fb SUS-13-013 L=19.5 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-13-003 L=19.5 9.2 /fb SUS-12-027 L=9.2 /fb SUS-13-003 L=19.5 9.2 /fb SUS-13-003 L=19.5 /fb EXO-12-002 L=4.8 /fb SUS-12-027 L=9.2 /fb SUS-12-027 SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb SUS-12-027 L=9.2 /fb EXO-12-049 L=19.5 /fb Summary of CMS RPV SUSY Results* of CMS RPV Summary 0 231 231 112 122 123 233 233 112 122 123 233 233 333 122 123 233 233 112 323 ' ' ' ' ' ' ]. '' '' '' '' λ λ λ λ λ λ λ λ λ λ λ λ λ λ λ 6 λ λ λ λ

113/223

t t t '' ν ν ν ν ν ν Summary plot for R-parity violating CMS searches. The corresponding ATLAS results are similar. µ τ µ µ µ µ ν ν ν λ τ τ e b qll qll qll qll qll qll µ µ tbs µ tbt

qbt qqq qbt qbt qbt → → → → → → →

qqqq qqqq →

→ t ~ → → →

→ → If R-parity is violated, new terms For top squarks the situation is even more complex because of the many different decay chains Pair production of chargino, neutralinos, and sleptons at the LHC, for masses of several hun- Further results of SUSY searches can be obtained from the public result pages of ATLAS [ → → →

q ~ q ~ q ~ ~ g ~ g ~ g

qqb

~ g → → R R ~ q R ~ g ~ g ~ q R g ~ t ~ t t *Observed limits, theory uncertainties not included Only a selection of available mass limits Probe *up to* the quoted mass limit ~ t ~ ~ → R ~ g

~ q ~ g and CMS [ 3. Summary of R-parity violating searches that must be considered.also While regions in in the SUSY best parameterhundred case space GeV cannot limits where be of even ruled for up out light by to the neutralinos 700 LHC top GeV searches. squarks are abovedreds possible, a of there few GeV, are is attop least squark two pair orders production). of Therefore, magnitudeSUSY high smaller statistics particles. than data samples for Today, are coluored depending requiredaround SUSY on 700 to particles GeV constrain the in (e.g. these assumed the most scenario optimistictopologies. case limits Much to more on only data a these will few particles hundred be GeV needed vary for to from more push pessimistic these decay limits above the 1 TeV scale. Figure 3: degeneracy for first and second generationbe squarks. light, If, this however, only limit a weakens single tonos. squark only is For the assumed production to of singlebetter bottom control squarks of the the best SM limit background improves to via around the 650 identification GeV of due b to quarks in the final state. Searches for Supersymmetry PoS(EPS-HEP 2013)161 = 7, 8 TeV 1208.4688 1209.0753 1304.6310 1308.2631 1212.1272 1211.1167 1308.2631 1212.1272 1308.1841 1210.4826 1308.1841 Preliminary s Reference √ 1208.4305, 1209.2102 ATLAS-CONF-2013-062 ATLAS-CONF-2013-065 ATLAS-CONF-2013-089 ATLAS-CONF-2013-058 ATLAS-CONF-2013-047 ATLAS-CONF-2012-144 ATLAS-CONF-2012-140 ATLAS-CONF-2013-037 ATLAS-CONF-2013-025 ATLAS-CONF-2012-147 ATLAS-CONF-2013-036 ATLAS-CONF-2013-024 ATLAS-CONF-2013-068 ATLAS-CONF-2013-047 ATLAS-CONF-2013-048 ATLAS-CONF-2013-061 ATLAS-CONF-2013-061 ATLAS-CONF-2013-049 ATLAS-CONF-2013-061 ATLAS-CONF-2013-057 ATLAS-CONF-2012-147 ATLAS-CONF-2013-025 ATLAS-CONF-2013-007 ATLAS-CONF-2013-051 ATLAS-CONF-2013-028 ATLAS-CONF-2013-069 ATLAS-CONF-2013-036 ATLAS-CONF-2013-007 ATLAS-CONF-2013-093 ATLAS-CONF-2012-152 ATLAS-CONF-2013-035 ATLAS-CONF-2013-047 ATLAS-CONF-2013-062 ATLAS-CONF-2013-092 ATLAS-CONF-2013-049 ATLAS-CONF-2013-026 ATLAS-CONF-2013-035 ATLAS-CONF-2013-091 ) 1 ± 1 ˜ χ − )) )) )) )) ˜ g m( 0 1 0 1 0 1 ˜ ˜ χ χ ˜ χ << ) )=108 GeV ATLAS )+m( 1 0 1 0.2 ns 0 1 t ˜ )+m( )+m( )+m( ˜ χ ˜ χ ± 1 1000 s ± 1 ± 1 )= ˜ χ ˜ χ ˜ )=5 GeV χ < ± 1 ) 0 1 ˜ χ ˜ χ g -type are between ( (˜ Oliver Buchmueller τ )=1, m( 00 687GeV for D8 0 <τ µ )=0.5(m( )-m( s 0 < > ± ± 1 )=0.5(m( )=0.5(m( µ )=0.5(m( > 1 mm ˜ ˜ χ χ )=0% )=0, sleptons decoupled )=0, sleptons decoupled ν )-50 GeV, m( ν ν 0 1 0 1 121 c < ,˜ ,˜ λ ,˜ =0.05 ˜ ℓ ˜ ˜ χ χ λ 133 τ ˜ ℓ ˜ W λ =0.05 LSP 160 MeV, ) τ 85 GeV = (4.6 - 22.9) fb 0 1 = )-m( 132 1(2)33 ), m( ), m( c )=BR( Mass scale [TeV] < ˜ χ eV ) )+180 GeV 2 ns 1 0 2 0 2 ) λ λ b 0 1 0 1 t ˜ ), ) < 4 0 1 ˜ ˜ 50 χ χ )=0, m( ˜ ˜ χ χ 156 mm, BR( ) − ˜ ˜ ˜ 0 1 χ g g dt ) ) 0 1 350GeV 0 GeV ˜ χ 200GeV, m( 50GeV 300 GeV, 50GeV 200GeV, m( 400 GeV 220 GeV 300 GeV 90GeV 80 GeV, 600 GeV 150 GeV β< ˜ ˜ ˜ 200 GeV q q χ τ< 18 10 < 80 GeV, limit of 15 ( < > > > < < > = < < > < > > c )-m( )=m( )=m( )=2 m( ) )=0 GeV ) ) )=0 GeV ) ) =m( ) )=0 GeV )=55 GeV )=0 GeV )=0 GeV ) )=0 GeV, m( ) )=100 GeV, 10 ) ) )=0 GeV ) ) ) )=0 GeV, m( ) ) )=BR( > L < )-m( )=m( ) ) =0.10, =0.10, )=m( )=m( tan 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 1 ± 1 ± 1 0 1 ± 1 0 1 0 1 0 1 0 1 0 1 0 1 ± 1 0 1 0 1 0 1 0 1 0 1 ) 0 1 t < 1 1 <τ β> β< ˜ ), m( R ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ χ q χ χ χ χ χ q χ t t H g ˜ ˜ < 0 2 ′ 311 ′ 311 ˜ χ m( m( m( m( 0.4 m( m( m( m( m( m( m( m( m( λ tan 10 any m( m( m( m( m( m( m( any m( m( m( m( m( m( m( λ m( m( m( m( m( m( 1.5 m( m( incl. limit from 1110.2693 m( tan m( m( BR( )=m( ± 1 ˜ χ m( 1.7 TeV 1.61 TeV 1.4 TeV 1 1.3 TeV 1.3 TeV 1.34 TeV theoretical signal cross section uncertainty. 1.2 TeV 1.2 TeV 1.2 TeV 1.24 TeV 1.18 TeV σ 1.1 TeV 1.1 TeV 1.1 TeV 1.12 TeV 1.07 TeV 1.0 TeV 916 GeV 900 GeV 880 GeV 832 GeV 800 GeV 760 GeV 740 GeV 704 GeV 690 GeV 645 GeV 619 GeV 600 GeV 320-660 GeV 100-620 GeV 200-610 GeV 500 GeV 150-580 GeV 475 GeV 225-525 GeV 271-520 GeV 125-450 GeV 275-430 GeV 350 GeV 315 GeV 285 GeV 85-315 GeV 5 180-330 GeV 270 GeV 100-287 GeV Mass limit 230 GeV 130-220 GeV 90-200 GeV 1 − 110-167 GeV 10 0 2 0 2 0 2 scale ˜ ˜ ˜ χ χ χ 2 , , , ˜g / 1 0 1 ± 1 ± 1 ± 1 ± 1 ± 1 ± 1 ± 1 0 1 ± 1 1 1 , τ τ 1 1 1 1 1 1 2 1 1 ] ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ sgluon t t t t t t t χ ˜g ˜g F ˜q ˜q ˜g sgluon M* scale ˜q ˜g ˜g ˜g ˜ b ˜ b ˜ ℓ q ˜g ˜q, ˜g ˜g ˜g ˜g ˜g ˜g ˜g ˜g ˜g ˜g ˜g ˜g t t χ χ ν χ χ χ χ χ χ ν χ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ 1 − dt[fb 4.8 4.8 4.6 4.8 4.6 4.6 5.8 r phenomena is shown. All limits quoted are observed minus 1 10.5 20.7 15.9 20.3 10.5 20.3 20.3 20.3 20.3 20.3 20.3 20.1 20.7 14.3 20.7 20.7 22.9 20.3 20.1 20.3 20.7 20.7 20.7 20.1 20.7 20.3 20.1 20.3 20.7 20.3 20.3 L R -type couplings connect the two. 0 - - - miss T Yes 20.3 Yes Yes Yes 4.7 Yes 20.3 Yes 4.7 Yes Yes 20.7 Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes Yes 20.3 Yes Yes 20.3 Yes Yes 20.1 Yes Yes Yes 20.7 Yes Yes Yes 4.7 Yes Yes Yes Yes 20.5 Yes Yes Yes 4.7 Yes Yes E λ -tag = 8 TeV c b b b s b b b b b b b b b b b b full data ------0 0 0 0 √ 2 3 1 1 1 3 2 1 2 3 1 2 0-3 0-3 1-2 7 jets 2 jets 4 jets 3-6 jets 0-2 jets 2-6 jets 2-6 jets 2-4 jets 3-6 jets 2-6 jets 1-5 jets 0-2 jets 0-3 jets 6-7 jets Jets 7-10 jets 7-10 jets mono-jet mono-jet mono-jet/ γ ) 0-3 jets ) ) τ τ γ , µ µ µ Z Z Z -type couplings appear between lepton superfields only, + + µ + µ µ µ µ µ µ µ µ µ µ µ µ µ µ ( , , , ( ( τ µ τ (SS) (SS) (SS) , , , , , , , , , , , , , , , τ γ γ e e e µ µ µ µ µ µ 0 0 γ 0 0 0 0 0 0 0 0 0 0 0 0 0 e e e e e e e e e e e e e e e , µ µ µ , , , 2 2 , 2 , , , , , λ 1-2 1-2 e e 1 2 1 1 3 2 2 2 1 2 3 4 2 1 2 e e e e µ e e e , displ. vtx 0-1 1-2 0-1 1 3 1 = 8 TeV 3 2 µ ) 2 2 2 Disapp. trk 1 jet µ s e, 1 , e τ √ e ν ˜ ν partial data ˜ ( ± 1 µ ) τ τ τ ˜ χ e 0 1 χ e ¯ q + t ¯ , ) , ˜ ) χ q t µ µ e µ )+ ν νν ˜ ν ˜ , ˜ → → µ (˜ + 0 1 e ( ℓ ee ττ shows a summary of R-parity violating SUSY searches from CMS. The correspond- (˜ 0 1 ˜ χ e e L ± 1 τ ˜ 0 1 ˜ χ ˜ ℓ ± → → ˜ χ 0 1 ˜ ) χ ν → → ˜ 0 1 0 1 0 1 0 1 → b t τ τ ℓ ˜ χ R-hadron ˜ ˜ χ χ 0 1 ˜ ˜ χ χ 3 ν ν ± 1 ) ) , , t t ), ˜ , ˜ , ˜ χ → → ˜ χ ˜ ν g ˜ ν 0 1 0 1 ˜ = 7 TeV , long-lived qqW 1 1 0 1 , 0 1 b Wb τ ℓ X X ˜ ˜ χ χ t t 0 1 νν → → ˜ ˜ Z τ ˜ ˜ χ ˜ χ ( ˜ ( s G (˜ 1 1 ˜ χ 0 1 → full data (RPV) ± 1 → → ℓ t t Summary table for the ATLAS searches. The corresponding summary from CMS is very similar. prod., long-lived ˜ ˜ γ Z h bs ℓ + + 0 1 √ 0 1 ˜ χ + ± 1 ˜ τν W W ℓν ˜ ˜ 1 1 χ ℓℓ/ℓν/νν L µ 0 1 0 1 ˜ ˜ t t χ τ τ χ ˜ ˜ ˜ − 1 χ ( b t ˜ ℓ 1 0 1 → → → ˜ ˜ χ χ ν ν → → → → ˜ ˜ NLSP) NLSP) c t ¯ ˜ ν q χ ˜ . The plot shows exclusion mass limits of ATLAS for different searches and interpretation ˜ 0 1 ˜ χ ℓ 1 qq → → L t + 1 + 1 + 1 + 1 q qq qq ˜ ˜ ˜ ℓ ℓ ˜ 0 1 χ + 1 , q + 1 → → ˜ 1 1 W W ℓ 0 1 0 1 → → ˜ ˜ ˜ ˜ , χ χ χ χ ˜ ˜ χ χ → ˜ 4 χ 1 2 ˜ ˜ b b ˜ ˜ χ χ t → → → , , , , → 0 1 t t ¯ ˜ ˜ b t ¯ → → → L,R t t , , pp pp ¯ ¯ 1 ˜ ˜ ˜ g g g − 1 − 1 − 1 − 1 ˜ ˜ χ q (medium), (heavy), (heavy), , (natural GMSB) , (light), (light), (medium), ˜ ℓ 0 2 0 2 0 2 t qqq t b b t 1 1 ˜ , , , ˜ ˜ ˜ ˜ χ χ χ χ 1 1 1 1 1 2 1 1 1 , , ˜ ˜ ˜ χ χ χ ˜ ˜ Model b b t t t t t t t t t ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜

˜ ˜ ˜ g g g → → → → → → ˜ ˜ q q + 1 + 1 + 1 + 1 ± 1 ± 1 ± 1 1 1 L,R 1 1 1 1 1 2 1 1 1

˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ The interpretation of results at the LHC has moved away from constrained models like the A comprehensive overview of the current landscape of SUSY searches at the LHC is given in Figure ˜ WIMP interaction (D5, Dirac Direct Stable, stopped GMSB, stable GMSB, LFV LFV Bilinear RPV CMSSM Scalar gluon pair, sgluon Scalar gluon pair, sgluon MSUGRA/CMSSM MSUGRA/CMSSM GMSB ( GMSB ( GGM (bino NLSP) GGM (wino NLSP) GGM (higgsino-bino NLSP) GGM (higgsino NLSP)Gravitino LSP 2 MSUGRA/CMSSM ℓ t t t t t t q χ χ b b t t t χ χ χ χ χ q g g g g g g g g g ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜ ˜

direct

˜ g particles med. ietproduction direct

RPV Other nlsv Searches Inclusive

3 3

EW e.squarks gen. gen.

ATLAS SUSY Searches* -Status: 95% CL SUSY Lower Limits 2013 Long-lived

rd rd *Only a selection of the available mass limits on new states o Figure 4: CMSSM towards a large setNew of Physics has simplified been models, observed0.5 or at the TeV the to pMSSM. LHC. 1.4 So Limitscorresponding far TeV on decay depending no coloured chains. significant on SUSY sign the Limits particleshold of assumptions on range for made third between light for generation neutralinos, underlying squarksSUSY and production below and are the modes electroweak 1 all gauginos and TeV well scale only is below certainly the not 1 yet ruled TeV out. mass scale. Therefore. in general, assumptions. The corresponding results from CMS are comparable. ing ATLAS summary is similar. It isexperiments already interesting to probe note the that 1 for TeV scale. many different signatures the LHC 4. Summary Figure generation indices; quark superfields only, and Searches for Supersymmetry PoS(EPS-HEP 2013)161 D86 (2008) 3 JINST Phys.Rev. , Oliver Buchmueller (2008) S08004 3 JINST , , in: 2010 Review of Particle Physics (Particle Data 6 13 TeV or higher will increase the production cross = s √ Experimental review of searches for Supersymmetry (see also , in: 2012 Review of Particle Physics (Particle Data Group) The ATLAS Experiment at the CERN Large Hadron Collider , 075021 (2010). The CMS experiment at the CERN LHC G37 Supersymmetry, Part II (Experiment) J. Phys. S08003 September 2013 Update) 010001 (2012). Group), https://twiki.cern.ch/twiki/bin/view/CMSPublic/PhysicsResultsSUS https://twiki.cern.ch/twiki/bin/view/AtlasPublic/SupersymmetryPublicResults The forthcoming run of the LHC at [1] CMS Collaboration, [2] ATLAS Collaboration, [3] O. Buchmueller and P. De Jong, [4] J.-F. Grivaz, [6] CMS public results on SUSY searches: [5] ATLAS public results on SUSY searches: section for SUSY particles substantially andery. will thus present again a great opportunity for discov- References Searches for Supersymmetry