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Supersymmetry at HERA
Motivation for SUSYBasic SUSY factsDifferent SUSY modelsCurrent limitsSparticle creation at HERASUSY analyses at ZEUSFuture prospects
DESY Student Seminar, 14.Nov.2005
Claus Horn
SUSY at HERA, 14.Nov.2005 Claus Horn
Shortcomings of the Standard Model
SM is only low energy approximation,In a fundamental theory all interactions should be unifiedGUT + gravity
What is the origin of mass,Introduction of Higgs boson runs into problems.
Cosmological problems
21 parameters – too many!Why three generations ?Why |Qel| = |Qp| ?...
SUSY at HERA, 14.Nov.2005 Claus Horn
Motivation for Supersymmetry
• Coleman-Mandula theorem • Unification of the forces • Solution of the Hierarchy problem • Candidates for dark matter • Necessary for quantum-gravity
SUSY at HERA, 14.Nov.2005 Claus Horn
Coleman-Mandula Theorem
„In a theory with non-trivial scattering in more than 1+1 dimensions, the only possible conserved quantities that transform as tensors under the Lorentz group are the generators of the Poincare group and scalar quantum numbers.“
SUSY is the only possibel extension of the Poincare group.
Our last chance to discover a fundamental space-time symmetry!
Tensors fulfill comutation relationsAdd anti-commutators
Graded Lie-algebras„super algebra“
P: Energy-momentum operatorQ: Supercharge
SUSY at HERA, 14.Nov.2005 Claus Horn
Unification of the Forces
Renormalisation Group Equations describe running of the coupling constants due to screening / antiscreening
SM MSSM
Example:
Slope depends on number and masses of particlesin the model
Miracle!
SUSY at HERA, 14.Nov.2005 Claus Horn
Solution of the Hierarchy ProblemCorrections to the Higgs mass:
Contributions of particles arecanceled by contribution of theirsuperpartners.
SM:
MSSM:
Cancelation requires fine tuning to 17 orders of magnitude!
SUSY at HERA, 14.Nov.2005 Claus Horn
For unbroken SUSY: No quantum correction to the Higgs mass (mH=0).
Broken SUSY: “running” Higgs mass
superpartners have to be lighter than 1 TeV
SUSY exact
Q²SUSY particles
No SUSY
mH
mh
SUSY Higgs sectorvery restricted:
mh < 150 GeV Q2
SUSY at HERA, 14.Nov.2005 Claus Horn
Basic Facts about SUSY
Symmetry between fermions and bosons
Q|boson> = |fermion> Q+|fermion> = |boson>
No superpartners with same masses are observed.SUSY is a borken symmetry.
Spontaneous SUSY breaking in SM sector not possiblesupertrace theorem sum rules between particle andsparticle masses, e.g.: excluded!
Hidden sector models
SUSY at HERA, 14.Nov.2005 Claus Horn
Supermultiplets
Chiral supermultiplets: (fermion,sfermion) = (spin ½, spin 0)
Vectorial supermultiplet: (gauge boson, gauginos) = (spin 1, spin ½)
SUSY at HERA, 14.Nov.2005 Claus Horn
Sparticles of the MSSM
Neutral gauginos mix to form four neutralinos.
Charged gauginos mix to form two charginos.
M depends on M2, tan() and . BRs of 0 and
SUSY at HERA, 14.Nov.2005 Claus Horn
Parameters of the MSSM
• mA : pseudoscalar Higgs boson mass
• tan() : ratio of VEV of two Higgs doublets
• : Higgs mixing parameter
• M1, M2, M3 : gaugino mass terms
• All sfermion masses
• Ai: all mixing parameters of squark and slepton sector
SUSY at HERA, 14.Nov.2005 Claus Horn
SUSY BreakingMSSM does not explain origin of SUSY breakingsoft breaking terms are introduced „by hand“
more than 100 free parametersHidden sector models: mSUGRA, GMSB
Flavour problem solved in GMSB model.
SUSY at HERA, 14.Nov.2005 Claus Horn
minimal SUperGRavity (mSUGRA)
Parameter: m0, m1/2, A0, tan(), sign()
• Unified masses at the GUT scale m0: common scalar mass m1/2: common gaugino mass
• Unified trilinear couplings = A0
• Radiative EW symmetry breaking
Constraints:
M(G~) 1 TeV (in AMSB 10 TeV)
SUSY at HERA, 14.Nov.2005 Claus Horn
Gauge Mediated SUSY Breaking (GMSB)
Possible NLSPs: neutralino, stau
LSP (in not-yet excluded parameter space) is always gravitino
Distinct event signature: photon/tau + missing energy
Gravitino might be candidate for dark mattereven in RPV models.
Gravitino can be very light:
Parameter: , sqrt(F), Mmess, N, tan(), sign()
Very predictive mass spectrum, easy to distinguish from SUGRA.
SUSY at HERA, 14.Nov.2005 Claus Horn
Typical Mass Spectra
Neutralino1 is light(est)Next: right-handed slepton (stau) & chargino1
Squarks are relatively heavy
SUSY at HERA, 14.Nov.2005 Claus Horn
R-parity
Multiplicative discrete symmetry: RP=(-1)3B+L+2S+1 for SM particles -1 for sparticles
Most general Lagrangian contains additional trilinear terms in superpotential which violate RP:
HERA is the ideal place to look for ‘ !
(Proton decay only if ‘ and ‘‘ are 0 at the same time.)
RPC: sparticles pair-produced, LSP stable
SUSY at HERA, 14.Nov.2005 Claus Horn
Overview of current best Limits
• Neutralinos / Charginos RPC and RPV • Sleptons RPC and RPV• Squarks RPC and RPV
Huge multidimensional parameter spaces
Comparison between different analysis difficult.
Results only valid under restricted conditions.
SUSY at HERA, 14.Nov.2005 Claus Horn
Current best Limits
Neutralinos / CharginosParameter region:
LEP m(> 92GeV RPC MSSM m(> 103GeV tan()=2, =-200
D0 m() > 84 GeV RPV mSUGRA m() > 160 GeV tan()=1.5
LEP m(> 40GeV RPV MSSM m(> 103GeV tan()=1.5
SUSY at HERA, 14.Nov.2005 Claus Horn
Current best Limits - sleptons
selectronR > 100 GeVsmuonR > 95 GeVstauR > 86 GeV
LEP: RPC MSSM= -200 tan() = 1.5
D0: m(~) > 460 GeV 132=0.05 & ‘311=0.16
selectronR > 100 GeVsmuonR > 98 GeVstauR > 97 GeV
LEP: RPV MSSM = -200 tan() = 1.5
SUSY at HERA, 14.Nov.2005 Claus Horn
Current best Limits - squarks
D0: m(g~) > 232 GeV
D0: m(q~) > 320 GeV
RPC
mSUGRA m0 = 25 GeV
mSUGRA m0 = 500 GeV
SUSY at HERA, 14.Nov.2005 Claus Horn
Current best Limits - squarksRPV
CDF m(t~) > 155 GeV ‘3330HERA m(t~) > 275 GeV ‘1j1=0.3
SUSY at HERA, 14.Nov.2005 Claus Horn
Sparticle Creation at HERA
Systematic approach needed to filter all interesting channels.
Particles are produced on-shell (same for all SUSY models).Decay depends on sparticle spectra of SUSY model.
HERA topologies Abstract notation
SUSY-flow graphsFundamental vertices} Abstract diagrams
Approach:
SUSY at HERA, 14.Nov.2005 Claus Horn
HERA Topologies• All topologically distinct graphs with up to three outgoing (s)particle lines• Initial state is fixed to electron+quark (g and from proton are only considered with 2 outgoing lines)
SUSY at HERA, 14.Nov.2005 Claus Horn
SUSY-flow Graphs
Number of SUSY propagatorsNumber of SUSY particles
discarded
Choos RPV verticesMark sparticle lines with a „~“. In the case of RPC: C-like loops result.
F, RPC:
SUSY at HERA, 14.Nov.2005 Claus Horn
Abstract Notation & Fundamental VerticesPhysics description on an abstract level to reduce complexity.
All vertices of the MSSM ! (neglecting pure bosonic SM vertices)
SUSY at HERA, 14.Nov.2005 Claus Horn
Restrictions
• diagrams with > 3 on-shell produced (s)particles are neglected• diagrams with outgoing , g, Z0 are not discussed• diagrams with initial g/ and 3 outgoing particles are discarded• u-channel diagrams are not stated expicetly• diagrams with > 1 sparticle propagator are discarded• interactions of Higgs bosons are not considered• vertices with only SM bosons are neglected• diagrams with three RPV vertices are discarded
SUSY at HERA, 14.Nov.2005 Claus Horn
Example: Application to type C DiagramsRPC:
RPV:SUSY-flow graphs:
SUSY at HERA, 14.Nov.2005 Claus Horn
C3: disfavoured due to high limits on squark massesC7: - “ –C6: lepto-quark search / contact interactionC5: beeing analysed at the moment !
Possible abstract diagrams:
SUSY at HERA, 14.Nov.2005 Claus Horn
Sparticle Decays Neutralino:
RPC MSSM RPV MSSM GMSB
Chargino:
Stable LSP
missing energy
RPC RPV
SUSY at HERA, 14.Nov.2005 Claus Horn
Sparticle DecaysSleptons:
Squarks decay in the same way.
RPC MSSM: missing E, e / /RPV MSSM: 2 jets / 2 l / 2jets+2l GMSB: l + + G~
RPC: RPV:
SUSY at HERA, 14.Nov.2005 Claus Horn
ResultsDiagrams with squarks are neglected.
Characteristic signatures for different models!
SUSY at HERA, 14.Nov.2005 Claus Horn
Results
With two outgoing lines: C5With three outgoing lines and one sparticle: F4-2With three outgoing lines and two sparticles: D1
SUSY at HERA, 14.Nov.2005 Claus Horn
Interesting SUSY Diagram D1
Highest expected cross section for:• = • Low Q2 (PhP)
Calculated cross section: 20 pb for m=me~=120 GeV (no warrenty!)
• Only SM propagators • Production of two sparticles with m100 GeV each
Signature:RPC MSSM: E + e-
RPC GMSB: e-+2(+G~)
SUSY at HERA, 14.Nov.2005 Claus Horn
Interesting SUSY Diagram F4-2
Highest expected cross section for: resolved PhP
Cross section: to be determined
Signature:RPV MSSM: 2jets / 2jets+2lRPV GMSB: l+G~ / l++G~
• Only SM propagators• Only one sparticle • Slepton production (first time at HERA)
SUSY at HERA, 14.Nov.2005 Claus Horn
Current Analyses at ZEUS
Decay in MSSM:Gaugino analysis
Decay in GMSB:Gravitino analysis
'
Production via C5
NC-like channel
CC-like channel
Signature:
e- + jets
+ jets
jet + + missing energy
SUSY at HERA, 14.Nov.2005 Claus Horn
Gravitino Analysis
SUSY at HERA, 14.Nov.2005 Claus Horn
Discriminant Method
Box size
All events get classified.Less statistics needed.Faster calculation.More accurate results.Generally better S/B seperation.
Improvement: variable box size
Multidimensional cuts generallyresult in a better S/B ratio, than one dimensional cuts.
DS
S B
# events /box ~ (box_size)d
SUSY at HERA, 14.Nov.2005 Claus Horn
Gravitino Analysis
No events in signal region
SUSY at HERA, 14.Nov.2005 Claus Horn
Limits – Gravitino Analysis
SUSY at HERA, 14.Nov.2005 Claus Horn
Limits – Gaugino Analysis
Extended LEP limits in M2 - plane:
SUSY at HERA, 14.Nov.2005 Claus Horn
Future: LHC and ILC
SUSY at HERA, 14.Nov.2005 Claus Horn
Future Prospects - LHC
SUSY gauge couplings are the same as in SM.Cross sections only surpressed by mass terms.At high energies production rates should be similar to SM!
Discovery is no problem. (reonstruct Meff)
SUSY signal and SM bkg. for tt- decay (m0=1TeV, m1/2=500 GeV)
SUSY at HERA, 14.Nov.2005 Claus Horn
SUSY at LHC
Complicated decay channels: g~ -> q~q -> qq -> l~lqq -> llqq
Problem is to seperate different SUSY channels.
But:
LHC 5 discovery curves
SUSY at HERA, 14.Nov.2005 Claus Horn
Future Prospects - ILCHigher luminosity at similar energy
Precision measurements of SUSY parameters!
LHC:
ILC:
SUSY at HERA, 14.Nov.2005 Claus Horn
Future
SUSY at HERA, 14.Nov.2005 Claus Horn
Summary
• SUSY is a very interesting and promising theory.
• It is challenging, but there are SUSY channels were HERA is favoured compared to LEP and the Tevatron.
• If we do not find it before, then the LHC will give the final answer: Be prepared to discover a new world !