Physics Potential of the High Energy e+e- Linear Collider

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Presentation transcript:

Physics Potential of the High Energy e+e- Linear Collider Grahame A. Blair Royal Holloway, Univ. of London/DESY ASI Praha, 12 July 2003 Introduction to the machines Physics working groups Higgs Supersymmetry Extra dimensions Summary

The Machines JLC,NLC, TESLA, CLIC are all projects for a linear e+e- machine: JLC-X/NLC 0.5-1 TeV copper cavities operating at 11.4 GHz. TESLA 0.5-0.8 TeV superconducting Niobium cavities operating at 1.3 GHz CLIC 0.5-3 TeV copper cavities operating at 30 GHz See ILC-TRC megatables for detailed overview: http://www.slac.stanford.edu/xorg/ilc-trc/2002/2002/report/03rep.htm

LC for this talk: Also possible/important; Compton scattering to e+e- collisions with √s tuneable 0.5 – O(1) TeV e-e- mode. Polarisation: e- 80% (L/R); e+ 60% (?). Possiblity to run at √s ~ 90 – 160 GeV (“GigaZ”) Luminosity 3-6.1034 cm-2 s-1  specific analyses can assume up to about 1 ab-1 Also possible/important; Compton scattering to produce  or e

Bunch Interactions e+ e- Increase in luminosity (×~2) Schulte Increase in luminosity (×~2) Beamstrahlung  Lumi. Spectrum

Luminosity Spectrum sharp peak approx same as ISR (tuned) – few % in tail for 0.5-1 TeV machines TESLA TDR

Precision Measurement of the Top Mass Precision measurement of fundamental particle properties The top quark is the heaviest: most sensitive to new physics Cross section (pb) Mtop=175 GeV 100 fb-1 per point Statistical Precision ~0.05 GeV 0.02% Etot(GeV) Martinez et al.

Initial State e-R e+L e-R R W-production suppressed s-wave production of charginos ~  sharp threshold Specific polarisations for specific couplings (eg SUSY) http://www.ippp.dur.ac.uk/~gudrid/power/ e-R s-wave production of selectrons ~  sharp threshold R Direct production of higgs

Worldwide LC Studies http://blueox.uoregon.edu/~lc/wwstudy/ http://blueox.uoregon.edu/~lc/alcpg/ http://acfahep.kek.jp/

Worldwide studies (2) http://www.desy.de/conferences/ecfa-lc-study.html http://clicphysics.web.cern.ch/CLICphysics/

Status of the studies TESLA TDR All the regions are well advanced with physics studies Many analyses use full simulation and reconstruction Worldwide, detector R&D collaborations are forming/ have formed. Increasing emphasis on systematics and on LHC/LC combined analyses. http://www.cpt.dur.ac.uk/~georg/lhclc/ The TESLA Technical Design Report, DESY-2001-011, March 2001. The JLC TDR http://lcdev.kek.jp/RMdraft/ The Case for a 500 GeV Linear Collider http://xxx.lanl.gov/abs/hep-ex/0007022

Particle/Machine Physics The LC will be a very challenging machine Particle physicists are taking part in machine studies Beam diagnostics and control Background estimates Design studies The particle physics programme now goes beyond “what comes out of the IP”.

HIGGS

Higgs Production For Mh~120 GeV, 500 fb-1, √s=350 GeV 80,000 Higgs TESLA TDR

Higgs Spin Threshold excitation curve determine spin 20 fb-1 per point TESLA TDR 20 fb-1 per point

Higgs Mass mh=120 GeV TESLA TDR mh=150 GeV 500 fb-1 at √s=350 GeV

Higgs Recoil Mass + h Z - Etot= 2 Ebeam Ptot = 0 500 fb-1, √s=350 GeV TESLA TDR

Higgs Mass Precision Mh(GeV) Channel Mh (MeV) 120 llqq 70 qqbb 50 combined 40 150 ll recoil 90 qq WW 130 180 100 80 500 fb-1, √s=350 GeV

Higgs Branching Ratios For mh=120 GeV h→ BR/BR bb 0.024 cc 0.083 gg 0.055 ττ 0.050 Battaglia

Higgs Width Production cross section TESLA TDR

Higgs Potential λ/λ=0.22 (statistical) for mh=120 GeV Requires 1000 fb-1 Muehleittner et al.

SUSY Higgs √s=800 GeV TESLA TDR L=500 fb-1 L=50 fb-1 M ~ 1 GeV

Supersymmetry

Supersymmetry To prove existence of SUSY: Need to discover the SUSY partners Every SM has a superpartner Spins of SM/SUSY partner differ by ½ Identical gauge quantum numbers Identical couplings Needs accurate measurements of Mass spectra, cross-sections, BRs, Angular distributions, polarisation asymmetries

SUSY Reference Points Work with Sugra SPS1a: M1/2=250 GeV M0=100 GeV A0=-100 GeV sign()=+ tan=10 Higgs gauginos sleptons squarks √s=1TeV √s=500 GeV

Mass Measurements 100 fb-1 Threshold scans chargino ~  slepton ~ 3 Martyn et al.

Endpoint Measurements √s=400 GeV L=200 fb-1  Both sparticle masses Martyn

SPS1a: LC Threshold LC Endpoint e-e- Threshold LHC+LC (Preliminary) Martyn, Polesello Porod, Zerwas, GB

Including width effects e-e- running Including width effects m~50 MeV for 4 fb-1 Freitas, Miller, Zerwas Feng, Peskin

Cross-Section Measurements For mSugra: M0=100 GeV M1/2=200 GeV tanβ=3 sign()=+ Using 2× 500 fb-1 at √s=800 GeV Choi et al.

Luminosity Budget Several running modes requried. Grannis et al. Several running modes requried. Input will already exist from LHC

Model-Independent Extrapolation Renormalisation Group Eqns Measure complete spectrum Extract soft SUSY parameters at EW scale Input measured masses, couplings into RGEs Extrapolate model independently to high scales

Extrapolation: gaugino Mi-1 GeV Porod, Zerwas, GB

Extrapolations sfermion mass terms Q (GeV) mSUGRA structure reconstructed Fine structure?

GMSB Mi2 Mm GMSB reconstructed Messenger Scale measured Q (GeV) Mm=200 TeV, Λ=100 TeV, N5=1, tanβ=15 sign()=+

GigaZ

GigaZ The LC can also provide high luminosity running at the Z-pole and at W-threshold Approximately 100 fb-1 per year Needs specific linac bypass design TESLA TDR

Unification of Gauge Couplings Improved measurement of GUT scale Heavy Threshold effects eg colour triplet higgs …

Consistency of SM variables Erler, Heinemeyer Hollick, Weiglein, Zerwas

Extra Dimensions

Extra Dimensions Generally soft Escapes into bulk  missing energy Assumes: P(e-) =80%; P(e+) 60%

Measuring number of Dims. Runs at two energies: Measures δ Tests √s dependence Wilson

Summary The linear collider will provide high precision measurements at high energy: Masses, chiral couplings, branching ratios… Together with LHC data, LC allows model-independent extrapolations to very high energy scales. Structure of the theory at GUT scale may be complex and require high precision to discover. Exciting overlap with LHC analyses complementary searches, constraints in cascades… Long term programme from O(1) TeV, GigaZ, , multi TeV … … and an exciting one!