1. Uppsala University Seminar CERN, 11 February 2010 Physics Opportunities with a Multi-TeV e + e  Collider M Battaglia University of California at Santa Cruz, Santa Cruz, CA Lawrence Berkeley National Laboratory, Berkeley, CA and CERN, Geneva

2. Achieving e + e  collisions beyond 1 TeV Two-beam Acceleration Scheme CLIC Laser Wakefield Acceleration

3. Cleaning Chicane First module INJECTOR CLIC Test Facility (CTF3) to demonstrate: drive beam generation RF power production two-beam acceleration and reliability of structures:

4. Physics Motivations for e + e  at and beyond 1 TeV Precision Study of Rare/Suppressed SM Processes : Higgs Sector: g H , g Hbb for intermediate M H, g HHH, g ttH Probe New Phenomena beyond LHC Reach : Precision study of EW observables Access New Thresholds at the Tera-scale : Identify nature of New Physics and its connection to Cosmology

5. Physics and Experimentation at and beyond 1 TeV Physics Signatures Experimental Issues Reach and Accuracy Is Particle Flow applicable to multi-TeV collisions ? Are the Forward Regions exploitable ? Is accurate Jet Flavour Tagging possible ? Independent of Physics Scenarios can we identify Physics Signatures most relevant to e + e  physics at 1 TeV and beyond ? Is the study of these Physics Signatures enabled by the Accelerator Parameters ? Is the Physics Reach complementary and supplemental to the LHC capabilities ? Is the signature e + e  Accuracy preserved at 1 TeV and beyond ?

6. Physics Signatures at Multi-TeV Missing Energy Final States Resonance Scan Electro-Weak Fits Multi-Jet Final States hep-ph/0103338

7. 0.1 TeV0.5 TeV How is physics changing from 0.2 to 3 TeV ? 3.0 TeV  (pb) for SM Processes vs. E cm (TeV)

8. Jet Multiplicity B Hadron Decay Distance MB, hep-ph/0103338 Parton Energy 0.20.51.03.0 (GeV)3264110240 Observables from 0.2 TeV to 3 TeV (SM Evts)

9. Precision Study of Rare/Suppressed SM Processes

10. The Higgs Boson and CLIC Flaecher et al. arXiv:0811:0009v2 WW fusion process offers significant cross section and benefits from high energies MB, De Roeck, hep-ph/0211207

11. g HHH BR(H  bb) BR(H   ) BR(H  gg) BR(H   ) E cm L 0.35 TeV 0.5 ab -1 0.50 TeV 0.5 ab -1 1.0 TeV 1.0 ab -1 3.0 TeV 2.0 ab -1 Pol: e  80% e  50% TESLA-TDR 2001 Kuhl, Desch, LC-PHSM-2007-001 Barklow, hep-ph/0312268 MB, DeRoeck, hep-ph/0211207 MB, J Phys G35 (2008) 095005 Barklow, hep-ph/0312268 The Higgs Sector at CLIC: Light Higgs Profile MB, LCWS08

12. Fermion Couplings: e + e   e e H 0  bb MB, De Roeck, hep-ph/0211207 Large WW fusion cross section yields samples of (0.5-1) x 10 6 H bosons; Gain in cross section partly offset by increasingly forward production of H, still within there is a 1.7 x gain at 3 TeV compared to 1 TeV.

13. MB, JPhys G35 (2008) Full simulation CLIC analysis based on ILC C++ software and SiD detector model: e + e   e e H      Fermion couplings: e + e   e e H   +  

14. The Higgs Sector at CLIC: Heavy Higgs Profile Recoil Mass in e + e  X for M H =600 GeV  (HH ) vs. g HHH Decay-independent Higgs observation and mass measurement in e + e   e + e  H 0 Possible sensitivity to triple Higgs coupling for heavy Higgs bosons CLIC promises to preserve LC signature capabilities for Higgs studies at large boson masses: MB, hep-ph/0103338

15. Experimental Issues MB, hep-ph/0103338   hadrons CLIC 1 BX Tag and measure ~250 GeV forward electrons in presence of   hadrons and pairs Simulation shows that background requires fast time stamping (O(10 ns)) and robust jet clustering ( anti-kt algorithm ) as adopted at LHC:

16. Access New Thresholds at the Tera-scale

17. Which is the scale of New Physics ? Waiting for LHC results, many attempts to define "most likely" region(s) of parameters based on LEP+Tevatron, low energy data and Cosmology (DM and BBN):

18. How Many Observable Particle ? MB et al., Eur Phys J C33 (2004) 0.5 TeV 1.0 TeV 3.0 TeV Ellis et al., PLB565 (2003)  h 2 and (g-2)  Constraints on cMSSM tan  = 10

19. Ellis et al., JHEP 0605 (2006) Which is the scale of New Physics ? 1) cMSSM with constraints and m 0 tuned to match  CDM h 2 at various tan  values tan  = 10 tan  = 50 cMSSM tan  = 35

20. Buchmuller et al., JHEP 0809 (2008) Which is the scale of New Physics ? 2) cMSSM with 15 constraints (EW, B physics, (g-2)  and  CDM h 2 ) 3) NUHM SUSY with 15 constraints (EW, B physics, (g-2)  and  CDM h 2 ) Most Probable Spectrum

21. Buchmuller et al., JHEP 0809 (2008) Which is the scale of New Physics ? 2) cMSSM with 15 constraints (EW, B physics, (g-2)  and  CDM h 2 ) allowed region largely extends towards high mass solutions

22. Cakir et al, hep-ph/0203121 4) In scenarios with gravitino LSP, long-lived staus may form metastables states with nuclei affecting Big Bang Nucleosynthesis ; These scenarios indicate very large sparticle masses, even too large for detection at LHC but well suited for CLIC: Which is the scale of New Physics ?

23. Allanach et al., PRD 73 (2006) CLIC 3 TeV SUSY Heavy Higgs Bosons: M A – tan  cMSSM ILC/CLIC 1 TeV

24. Ellis et al., JHEP 0502 (2005) SUSY Heavy Higgs Bosons: M A CLIC 3 TeV ILC/CLIC 1 TeV 1) cMSSM with constraints and m 0 tuned to match  CDM h 2

25. Allanach et al., JHEP 0808 (2008) CLIC 3 TeV SUSY Heavy Higgs Bosons: M A 5) String-inspired Large Volume Scenario SUSY with MCMC in Bayesian statistics formalism ILC/CLIC 1 TeV

26. DM A 0 Funnel Region LHC/ILC/CLIC Reach in M A – tan  DM A 0 Funnel Region CLIC 3 TeV

27. Lower energy LC Higgs data interpretation requires excellent control of parametric and theoretical uncertainties: Droll and Logan, PRD 76 (2007) SUSY Heavy Higgs Bosons: M A – tan 

28. Heavy Higgs Bosons: H at 3 TeV e  e   H + H   tbtb at 3 TeV Barrel ECAL Mokka SiD MB Large jet multiplicity gives particle overlaps in calorimeters. study distance (charged particle to closest cluster) (full G4 simulation) Coniavitis Ferrari, Pramana 69 (2007) CLIC 3 TeV

29. Heavy Higgs Bosons: H at 3 TeV e  e   H + H   tbtb at 3 TeV Coniavitis, Ferrari, PRD 75 (2007) M H =900 GeV

30. Analysis of 1 TeV events with ILC Detector Study e  e   HA  bbbb with LDC  CDM h 2 gives tight requirement of Heavy Higgs Bosons: H 0, A 0 at 1 TeV MB et al PRD 78 (2008) ILC 1 TeV

31. Analysis of 3 TeV events with CLIC-ILD Detector Study e  e   HA  bbbb with full G4 sim + reco Heavy Higgs Bosons: H 0, A 0 at 3 TeV MB et al, CLIC09 CLIC 3 TeV Coniavitis, Ferrari, Pramana 69 (2007)

32. Establishing the Nature of New Physics SUSYUED Given limited nb. of observable particles determine the nature of new physics: Example: tell UED from SUSY 1 TeV 3 TeV Tait and Servant

33. Establishing the Nature of New Physics MB et al, JHEP 0507 (2005) SUSYUED kinematics production angle

34. The LHC SUSY Inverse Problem Arkani Hamed et al, JHEP 0608 (2006) Given LHC data can we identify the nature of the underlying theory ? Study the inverse map from the LHC signature space to the parameter space of a given theory model: MSSM. 43026 models tested in 15-dim parameter space  283 pairs of models have indistinguishable signatures at LHC.

35. Solving the SUSY Inverse Problem at LC Berger et al, arXiv:0712.2965 Consider 162 pairs indistinguishable at LHC: only 52% (85 pairs) have charged SUSY particles kinematically accessible at 0.5 TeV, 100 % accessible > 1 TeV; 79% (57 out of 73 pairs) can be distinguished at 5  level at 0.5 TeV; 1-3 TeV data needed to extend sensitivity and solve the LHC inverse problem over (almost) full parameter space.

36. An UED Inverse Problem Bhattacherjee et al., PRD78 (2008) Mapping UED the parameter space from measurements at 1 TeV and 3 TeV linear collider:

37. Understand SUSY-Cosmology Connection Baltz, MB, Peskin, Wiszanski, PRD74 (2006) Dark Matter Density LCC1LCC2 8% LCC3LCC4 LC precision motivated by need to match  h 2 accuracy from CMB data ( ):

38. Mass Spectrum and e + e - Pair-Production Cross Sections

39. First determine dependence of Ωh 2 on sparticle masses by varying only parameter under study: Implications of the CLIC Accuracies: Neutralino Relic Density Ωh 2 in MSSM MB, CLIC09

40. ParticleMass Accuracy (GeV) ±1±1 ± 4.3 ±R±R ± 6.2 ±1±1 ± 6.7 e + e    + 1  - 1,  R  R,  1  1 Threshold Scans Threshold scans with 2 ab -1 at maximum energy and 2 ab -1 at 2.0-2.7 GeV MB, Blaising, CLIC09

41. Implications of the CLIC Accuracies: Neutralino Relic Density Ωh 2 in MSSM Perform scan to full MSSM imposing constraints on sparticle masses as obtained from preliminary CLIC analyses; Result SetdΩh2/Ωh2dΩh2/Ωh2 H 0 /A 0,  0 1,  ± 1, t 1,  R ±0.167 +  ± 2, t 2,  0 3 and  0 4 ±0.110 Preliminary ParticleMass Accuracy (GeV) ±1±1 ± 4.3 ±R±R ± 6.2 ±1±1 ± 6.7 0101 ± 4.0 H 0 /A 0 ±5.6 MB, Blaising, CLIC09

42. What if there is no Higgs ? Study strong interaction of W/Z bosons and identify resonance formation in the TeV region; Example 2 TeV resonance with 12 fb production cross section at 3 TeV, ~4 fb after acceptance cuts: including   hadrons De Roeck, Snowmass 2001

43. Experimental Issues ECal HCal Charged-Neutral Particle Distance in Calorimeters   hadrons background MB, CLIC2009 50 BX 850 Reco Trks in VTX

44. New Resonances at CLIC 5-point scan of broad resonance (3 TeV SSM Z') with ~ 1 year of data under two assumptions for luminosity spectrum (CLIC.01 and CLIC.02) Luminosity spectrum effect on mass and width reconstruction at CLIC: MB et al., JHEP 0212 (2002)

45. KK Resonances in ED Scenarios Observe interference between Z and  KK excitations accounting for CLIC luminosity spectrum: MB et al., JHEP 0212 (2002)

46. Probe New Phenomena beyond LHC Reach

47. New Physics beyond the LHC Reach Precision electro-weak observables in e + e   ff at 1- 3 TeV CERN-2004-005Grefe, CLIC08

48. New Physics beyond the LHC Reach: ED 5 TeV 3 TeV Reach for ADD model scale M s vs. integrated luminosity for 3 TeV and 5 TeV data: CERN-2004-005

49. New Physics beyond the LHC Reach: ED, Z' MB et al, hep-ph/0112270

50. New Physics beyond the LHC Reach: Contact Interactions MB et al, hep-ph/0112270

51. Experimental Issues Schulte. CLIC08 Perform precision tracking and vertexing accounting for beam stay clear and hit density from pair background; Optimise pixel size, bunch tagging,...

52. Theory Issues Anticipated experimental accuracy in determination of EW observables at and beyond 1 TeV, needs to be matched by theoretical predictions accurate at O(1%) to ensure sensitivity to New Physics; Beccaria, CERN-2004-005 Example: at 1 TeV W-boson corrections of the form amount to 19%. Electroweak radiative corrections include large Sudakov logarithms which will contribute sizeable uncertainties

53. Waiting for LHC results, there is a compelling case for vigorously pursuing a technology able to offer e + e  collisions at, and beyond, 1 TeV with high luminosity; Physics potential at 1 – 3 TeV appears very rich, preserving the signature e + e  features of cleanliness and accuracy represents a challenge, which needs a combined effort from physics benchmarking, detector R&D, machine parameter optimisation; Optimal balance between very high precision at high energy and high precision at very high energy can be assessed only with first LHC results at hand. For now enough to do tackling the issues above. CLIC offers unmatched energy range from 0.5 TeV up to 3 TeV making it an extremely appealing option for accessing the energy scale of LHC and beyond with e + e  collisions;