Searches for mSuGRA and related SUSY at LEP

Klaus Desch - Searches for mSuGRA and related SUSY at LEP - Boston 17/03/03 1/31

ALEPH DELPHI L3 OPAL

Klaus DeschUniversity of Hamburg

on behalf of the LEP collaborations

Northeastern UniversityBoston, 17/03/03

Why search for SUSY at LEP?

a posteriori reasoning:

• light Higgs boson:

SUSY prediction: at tree level in MSSM

• electro-weak mixing angle:

SUSY-GUT prediction of

h Zm mhm 135 GeV

hm 211 GeV (95%CL)

2W ssin ( )

2 SUSY GUTWsin 0.2335(17)

2 LEP / SLD

Wsin 0.2315(02)

could this be an accident???

from EW fit

How to search for the sparticles? q

,Z,h,HW ,H

q01 / 2 / 3 / 4

1 / 2g

many different sparticles

many different production mechanisms

many decay modes

depend on many (~105)

parameters (MSSM)

hopeless to perform a dedicated search for each configuration

strategy at LEP:

identify + classify topologies

perform searches as model-independent as possible

then use (possibly overlapping) subsets of the searches for the interpretation within a certain model

We don’t search for “mSuGRA”, etc. !

“Classic” SUSY Search Strategy

• LSP pair production not (really) visible: search for the NLSP, which may be a:

• charged slepton

• sneutrino (invisible, might be disturbing in decay patterns)

• squark (typically too heavy hadron collider, unless strongly mixed, stop, sbottom)

• chargino

• heavier neutralinos

• gluino (only higher order process in e+e-, hadron collider)

The LEP2 data sample

All four experiments ADLO have performed the basic searchesfor sleptons, squarks, charginos and neutralinos

LEP SUSY Working Group: combination of the results

http://lepsusy.web.cern.ch/lepsusy/

Especially important for the highest energies: ECM>207.5 GeV (ADLO=35.2 pb-1)

LEP combined sample:~ 2.6 fb-1

Search for Charged Sleptons

• Smuons: almost model-independent cross section

• Staus: mixing ( lighter stau can decouple from Z, reduced cross section)

• Selectrons: t-channel with neutralino exchange ( model dependent, usually constructive interference)

Signature: acoplanar lepton pairs

Main Background:

No mass reconstruction possible use multi-variate techniqueto exploit kinematical differences between signal and background(depends on assumed slepton mass)

e e W W

A typical smuon candidate (and background) event:

Numbers of observed events and expected background events:

any significant excess or deficit ?Calculate confidence level for excess/deficit using likelihood ratio method

Selected events are correlatedover wide areas in the plane

For a “true” signal, would expect significant excess over a wide area

No significant excess cross section upper limits

Cross section limits:

Selectrons: ~10 – 80 fb

Smuons: ~10 – 50 fb

Staus: ~40 – 150 fb

Except for the region with small

(few GeV) mass difference

Compare this again tothe MSSM predicted cross sections

mass exclusion almost up to kinematic limit possible

Charged Sleptons: Mass Limits

Only very weakly model-dependent

Search for Sbottom/Stop

In most (GUT-related) models, squarks are heavier than sleptons and charginos, unless there is strong mixing between L and R states.Off-diagonal elements of mixing matrix are ~ m(q) 3rd family LEP experiments concentrate on search for stop and sbottom

some experiments also look for4-body decay:

1 2 3 4e e tt bχ ff bχ ff

Production:

Decay:

ALEPH example of a multi-jet + missing energy event:

To make it short: no excess found in any of the 4 experimentsExclusion (partially complementary to Tevatron):

Example: 01b b

Mass limits (ADLO)

ALEPH: search for stable stop-hadrons:absolute limit on m(stop) > 63 GeVindependent of M

Search for Charginos

Production:

Decay:

Typical candidate in the channel

(but also compatible with WW)

• large cross sections up to kinematical limit

• universal cross section in Higgsino region

• model-dependency due to destructive interference with t-channel sneutrino exchange

Signal topolgy and SM backgrounds depend strongly on the mass difference

Large M: only moderate missing energySmall M: little visible energyVery Small M: lifetime effects

0M M( ) M( )

“Deep Higgsino region <<M2”

• Search for a wide grid in M(and and at many different is technically non-trivial

• Need (in principle) many millions of MC events

• Development of sophisticated interpolation techniques

• Increased sensitivity through modern selection techniques (likelihoods)

Example: input variables to hadronic chargino search in OPAL at s 206 GeV

Charginos: cross section limits

Single experiments:

100 fb for large part of mass plane

ADLO combination for highest energies:

1 pb even close to kinematical limit(104 GeV)

Chargino Mass Limit

M > 103 GeV M > 92.4 GeV

Mass limit for pure * 0

1W decays

Only somewhat weakened forlow M (see talk by A.Perrotta)

Interpretation of the Resultsin Specific Models

“Classic” SUSY searches are interpreted within:

None of the LEP2 searches for sparticles showed any significant excess exclusion limits in the parameter space of constrained SUSY models

CP odd Higgs massMA

Higgsino mixing parameter

Common trilinear couplingA0

Ratio of Higgs field v.e.v.’stan

Scalar mass at GUT scalem0

Gaugino mass at GUT scalem1/2

mSugra(4.5 parameters)

CMSSM“LEP”ConstrainedMSSM(6 parameters)

CMSSM exclusion

Exclusion in the m0-m1/2 plane:

Chargino2body Chargino

Chargino exlcusion weakly tan dependent but“light sneutrino” corridor (partially) covered by slepton searches

CMSSM LSP mass limit

LSP limit (in CMSSM) set by slepton searches in the corridor for large tan

Higgs tan exclusion depends on top mass (but not so critical for CMSSM LSP limit)

CMSSM Stau mixing

Mixing in stau sector canmake stau = NLSPCritical case: Small

Dedicated searches needed for

m m( ) m( )

0 0 0 02 1 1 1

and0 0 0 02 2 1 1

to recover sensitivity(Region III)

CMSSM Stau mixing

Preliminary ALEPHresult:

Stau mixing effectsdo not lower theCMSSM LSP limitfor tan2

mSuGRA InterpretationImpact of Higgs searches becomes larger (Higgs sector coupled tosparticle sector in mSuGRA)Exclusion in m0-m1/2 plane:

charginos

mSuGRA LSP Mass Limit

M(LSP) (any A0, mtop=175)

50.3 GeV

roughly: 1 GeV less per1 GeV larger mtop

Large tan: limit set by Charginos searches

Small tan: limit set by Higgs searches

Epilogue

PDG 2002: 25 years of SUGRA willhopefully be a real celebration!

…and then the real work (+fun) begins:How is SUSY broken: LHC + LC can find out

Special thanks to

G. GanisK. JakobsR. McPherson L. PapeC. RembserG. Sguazzoni

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