V.A. K hoze (IPPP, Durham & Manchester)

1. Studying the BSM Higgs sector by forward proton tagging at the LHC (Introduction) V.A. Khoze(IPPP, Durham & Manchester) (Based on works with S.Heinemeyer, A.Martin, M.Ryskin, W.J.Stirling, M.Tasevsky and G.Weiglein) main aim: to highlight recent development in the theory and phenomenology of the CED Higgs production

2. PLAN • 1. Central Exclusive Diffractive Production (only a taste). • Models and current understanding of uncertainties • (Dino, Alan, Misha, Jean-Rene) • 3. Prospects for CEDHiggs-boson production in BSM scenarios. • (VAK, Marek, Andy) . • 4. Physics backgrounds revisited. • 5. Conclusion.

3. (Khoze-Martin-Ryskin1997-2008) -4 (CDPE) ~ 10  (incl) New CDF results orders of magnitude differences in the theoretical predictions for the CEP of the Higgs are now a history

4. Visualization of QCD Sudakov formfactor arXiv:0712.0604 , PRD-2008 A killing blow to the wide range of theoretical models. CDF d

5. How reliable are the calculations ? Are they well tested experimentally ? ● How well we understand/model soft physics ? ● How well we understand hard diffraction ? ●Is ‘hard-soft factorization’ justified ? (Misha)  What else could/should be done in order to improve the accuracy of the calculations ? So far the Tevatron diffractive data have been Durham-friendly( Dino, Jim, Mike), (Alan,Misha) (Jean-Rene, Misha) or clouds on the horizon ?

6. Muchmore theoretical papers than the expected number of the CED produced SM Higgs events ‘Well, it is a possible supposition.’ ‘You think so, too ?’ ‘I did not say a probable one’

7. Survival of the Survival Factor Importance for the Forward Physics Studies at the LHC Serve as a litmus paper indicator of the level of our knowledge (theory & experiment) on diffractive physics at high energies Account for the absorption effects -necessitated by unitarity S² -a crucial ingredient of the calculations of the rate of the Central Excl. Diffractive processes +….. Prospects of New Physics studies in the Forward Proton mode (Alan, Misha) qualitativelynew stage •orders of magnitude differences in theoretical expectations – are a history (not so long ago-between Scylla and Charybdis) • new (encouraging) CED Tevatron results available, more results to come • we are discussing now the differences on the level of a factor of (3-4)

8. Selection Criteria for the Models of Soft Diffraction We have to be open-eyed when the soft physics is involved. Theoretical models contain various assumptions and parameters. Available data on soft diffraction at high energies are still fragmentary, especially concerning the (low mass) diffractive dissociation.   with a bit of personal flavour A viable model should: incorporate the inelastic diffraction :SD, DD (for instance 2-3 channel eikonal of KMR or GLM(M)) describe all the existing experimental data on elasticpp- scattering and SD ,DD and CED at the Tevatron energies and below (KMR; GLM(M), 0805.2799 ) be able to explain the existing CDF data on the HERA-Tevatron factorization breaking and on the CED production of the di-jets, di-photons, , J/, .., lead. neutr. at HERA provide testable pre-dictions or at leastpost-dictionsfor the Tevatron and HERA So far KMR model has passed these tests. Only a large enough data set would impose the restriction order on the theoretical models and to create a full confidence in the determination of S². Program of Early LHC measurements (KMR, M.Albrow et al.- FSC ) LET THE DATA TALK !

9. (Alan, Misha) -2000

10. (tot) , (el) , (SD) Bread and butter of TOTEM and ALFA measurements Importance forvarious LHC studies ( e.g. notorious Pile-Up) Low mass SD (DD)- one of the major current limitations on the models ( still not sufficient exp. Information) (Alan, Misha) KMR-07: relatively low (about 20% below the ‘standard’ central value)value of (tot) at the LHC ( S.Sapeta and K. Golec-Biernat-05) , (tot) 90 mb…cosmic rays, (early) LHC tests – coming soon inescapable consequence of the absorptive corrections caused by the higher-mass excitations GLM (arXiv; 0805.0418):(tot ) =110.5 mb, (el) =25.3 mb  (GLM)M (arXiv; 0805.2799):(tot ) = 92,1 mb, (el) =20.9 mb KMR (2007) (tot ) =90.5 mb, (el) =20.8 mb GLM(M)- essential improvement of their description of the Tevatron elastic and SD data

11. th

12. Are the early LHC runs, without proton taggers, able to check estimates for pp  p+A+p ? gap gap KMR: 0802.0177 Possible checks of: (i) survival factor S2:W+gaps, Z+gaps (ii) generalised gluon fg : gp Up Divide et Impera (iii) Sudakov factor T : 3 central jets (iv) soft-hard factorisation #(A+gap) evts (enhanced absorptive corrn)#(inclusive A) evts with A = W, dijet, U…

13. The main advantages of CED Higgs production • Prospects for high accuracy (~1%) mass measurements • (irrespectively of the decay mode). • Quantum number filter/analyser. • ( 0++dominance ;C,P-even) • H ->bb opens up (Hbb- coupl.) • (gg)CED bb inLO ; NLO,NNLO, b- masseffects - controllable. • For some areas of the MSSM param. spaceCEDP may become adiscovery channel! • H→WW*/WW - an added value (less challenging experimentally + small bgds., better PUcond. ) • New leverage –proton momentum correlations (probes of QCD dynamics , CP- violation effects…) H How do we know what we’ve found?  LHC : ‘after discovery stage’,Higgs ID…… mass, spin, couplings to fermions and Gauge Bosons, invisible modes…  for all these purposes the CEDP will be particularly handy !

14. without ‘clever hardware’: for H(SM)bb at 60fb-1 only a handful of events due to severe exp. cuts and low efficiencies, though S/B~1 . But H->WWmode at M>135 GeV. (B.Cox et al-06) enhanced trigger strategy & improved timing detectors (FP420, TDR) MSSM situation in the MSSM is very different from the SM SM-like > 4 generations:enhancedHbbrate (~ 5 times ) Conventionally due to overwhelming QCD backgrounds, the direct measurement of Hbb is hopeless The backgrounds to the diffractive H bb mode are manageable!

15. some regions of the MSSM parameter space are especiallyproton taggingfriendly (at large tan  and M , S/B ) KKMR-04 ; HKRSTW-07; B. Cox, F.Loebinger, A.Pilkington-07 (Marek,Andy) Myths For the channelbgds are well known and incorporated in the MCs: Exclusive LO - production (mass-suppressed) + gg misident+ soft & hard PP collisions. Reality The background calculations are still in progress : (uncomfortably & unusuallylarge high-order QCD and b-quark mass effects). About a dozen various sources (studied by Durham group)  admixture of |Jz|=2 production.  NLO radiative contributions (hard blob and screened gluons)  NNLO one-loop box diagram (mass- unsuppressed, cut-non-reconstructible)  ‘Central inelastic’ backgrounds (soft and hard Pomerons)  b-quark mass effects in dijet events ………..

16. A.G. Shuvaev & KMR.arXiv:0806.1447 [hep-ph] Further improvement of the g-b misidentification probability 1.3%0.5% or even better. In the CEP environment gbb could/should be menagable

17. The MSSM and more ‘exotic ‘scenarios If the coupling of the Higgs-like object to gluons is large, double proton tagging becomes very attractive (Andy,Marek) • The intense coupling regime of the MSSM (E.Boos et al, 02-03) CP-violating MSSM Higgs physics(B.Cox et al . 03,KMR-03, J. Ellis et al.-05) Potentially of great importance for electroweak baryogenesis • an ‘Invisible’ Higgs(BKMR-04) • NMSSM(J. Gunion, J.Forshaw et al.) • searches for the Higgs triplets (Andy)

18. New Tevatron data still pouring

20. (Marek) Mhmax benchmark scenario Improved theory & background 3 countours • “600X 2” scenario covers nearly the whole allowed region for the light Higgs. For large tan  heavy Higgs reach goes beyond 235 GeV. • For the H-boson the area reachable in the “60”-scenario is to large extent ruled out by the Tevatron data.

21. (Marek) CDM benchmarks (M. Tasevsky + HKRW) Compliant with the Cold DarkMatter and EW bounds (EHHOW-07) Tevatron limits • New bb-backgrounds TEVATRON 3 contours P3- NUHM scenario LEP limit

22. CDM P3 scenario 3  contours Abundance of the lightest neutralinio in the early universe compatible with the CDM constraints as measured by WMAP. The MA – tan planes are in agreement with the EW and B-physics constraints

24. at 220 GeV: CED (HWW/ZZ) rate – factor of ~9; at 120 GeV CED (Hbb) rate – factor of ~5. Simplest example of the BSM Higgs physics HZZ – especially beneficial

25. Experts claim that : Hints from B- factories Baryon asymmetry of the Universe Baryogenesis at the EW scale 4G is allowed by precision measurements 4G allows for the heavy Higgs 4G

26. for the light Higgs below 200 GeV

27. CDF & D0 At 60 fb-1 : for M=120 GeV , ~25 bb ev; for M=220 GeV, ~ 50 WW ev; favourable bgs, S/B>5

28. Conclusion Strongly suppressed and controllable QCD backgrounds in the forward proton mode provide a potential for direct determination of the Hbb Yukawa coupling, for probing Higgs CP properties and for measuring its mass and width. Insome BSMscenariospp p +(Hbb)+pmay become a discovery channelat the LHC. Further bgd reduction may be achieved by experimental improvements, better accounting for the kinematical constraints, correlations….. The complete background calculation is still in progress (unusually & uncomfortably large high-order QCD effects, Pile-Up at high lumi)

29. Backup

30. CURRENT EXPERIMENTAL CHECKS • ☻ Up to now the diffractive production data are consistent with K(KMR)S results • Still more work to be done to constrain the uncertainties. • Exclusive high-Et dijets • CDF:data up to (Et)min>35 GeV • ‘Factorization breaking’ between the effective diffractive structure functions measured at the Tevatron and HERA. • The ratio of high Et dijets in production with one and two rapidity gaps • CDF results on exclusive charmonium CEDP, (CDF to be submitted to PRL) • Energy dependence of the RG survival (D0, CDF). • Central Diffractive Production ofγγ (…., )(CDF, PRL-07) • ( in line with the KMRS calculations) ( 3 candidates & >10 more candidates in the new data) • Leading neutrons at HERA Dino, Mike  (PRD-2008)   LET THE DATA TALK ! Only a large data set would allow to impose a restriction order on the theoretical models

31. Mike Albrow (Fermilab) for the CDF 75+- 14

33. Approximate formula for the background c C~0.5 • M- mass window over which we collect the signal • b-jet angular cut : ( ) • bothSand Bshould be multiplied by the overall ‘efficiency’ factor • (combined effects of triggers, acceptances, exp. cuts, tagging efficienc., ….), •  ~4.2 % (120 GeV) • g/b- misident. prob.P(g/b)=1.3% (ATLAS) , P(g/b)0.5 % (new software) Four major bgd sources ~(1/4 +1/4 + (1.3)²/4 + 1/4 ) at M≈120 GeV, M= 4GeV