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1 1  V.A. Khoze ( IPPP, Durham ) (based on works by V.KHoze, M. RYskin and W.J. STirling and L. HArland-Lang ) Central Diffractive Production of Heavy.

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Presentation on theme: "1 1  V.A. Khoze ( IPPP, Durham ) (based on works by V.KHoze, M. RYskin and W.J. STirling and L. HArland-Lang ) Central Diffractive Production of Heavy."— Presentation transcript:

1 1 1  V.A. Khoze ( IPPP, Durham ) (based on works by V.KHoze, M. RYskin and W.J. STirling and L. HArland-Lang ) Central Diffractive Production of Heavy Quarkonia. (KHRYSTHAL collaboration)

2 2 Forward proton distributions and correlations. Tevatron, RHIC and LHC. CDP@LHC with FSC (topical examples ) With a bit of personal flavour

3 3 (star reactions!) New D0 jj- results RHIC, ALICE data expected Detailed tests of dynamics of soft diffraction (KMR-02) Spin-Parity Analyzer (KKMR -2003)

4 4,b,b

5 5 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 in LO ; NLO,NNLO, b- mass effects - controllable. For some areas of the MSSM param. space CEDP may become a discovery channel ! H → WW */ WW - an added value ( less challenging experimentally + small bgds., better PU cond. ) New leverage –proton momentum correlations ( probes of QCD dynamics, CP- violation effects… )  LHC : ‘after discovery stage’, Higgs ID …… H How do we know what we’ve found? mass, spin, couplings to fermions and Gauge Bosons, invisible modes …  for all these purposes the CEDP will be particularly handy ! CED Higgs production at the LHC

6 6 “soft” scattering can easily destroy the gaps gap eikonal rescatt: between protons enhanced rescatt: involving intermediate partons M soft-hard factoriz n conserved broken Subject of hot discussions recently : S² enh S²  absorption effects -necessitated by unitarity Everybody’s ~ happy (KMR, GLMM, FHSW, KP, S.Ostapchenco. Petrov et al, BH, GGPS, MCs..) (Beatriz)

7 7 ‘ Better to light a candle than to rant against darkness’ ( C onfucius ) Standard Candle Processes Standard Candle Processes

8 8 Our 3 measurements are all in good agreement (factor “few”) with the Durham group predictions. * * * Prpospects ! FSC@LHC (more coming soon )

9 9 CDF Collaboration, arXiv:0902.1271 [hep-ex], PRL KMRS -2004: 130 nb 80 nb (PDG-2008)  /KK mode as a spin-parity analyzer Prospects of  (b)-spectroscopy, FSC@CMS

10 10 (Currently no complete theoretical description of onium properties.) (BABAR (2008)) ( Still puzzles ) (spins- still unconfirmed) The heaviest and most compact quark-antiquark bound state in nature P-wave Bottomonia

11 11

12 12 Charmonium –like XYZ states

13 13 still unobserved

14 14 (maybe two different states X(3872), X(3875) )

15 15 What we expect within the framework of the Perturbative Durham formalism ( KMR-01, KKMR-03, KMRS-04, HKRS-10) Example, O++ -case *K NLO Strong sensitivity to the polarization structure of the vertex in the bare amplitude. Absorption is sizeably distorted by the polarization structure (affects the b-space distr.) KMR-02, KKMR-03, HKRS 09-10 KMR-01 Forward proton distributions& correlations- possibility to test diffraction dynamics KMR-02 (Gap size

16 16 Too good to be true ?! Phys.Rev.Lett.102:242001,2009

17 17 (HKRS-09,10)

18 18 (A. Alekseev-1958-positronium) (R.Pasechnik et al, Phys.Lett.B680:62-71,2009; HKRS, Eur.Phys.J.C65:433-448,2010 ) KMR-01

19 19 1 : 0.6 : 0.22 2

20 20 Spin-parity Analyzer

21 21 Central Diffractive Production of (Crystal Bal -1986) (about 0.25 of all hadronic decays (CLEO-2009)  (Barbieri et al (1979), NRQCD ) FSC@LHCb ? Suppressed non-resonant background 3 %.

22 22 1 : 0.03 : 0.08

23 23 Very topical for STAR@RHIC forthcoming measurements with tagged forward protons (new KHRYSTHAL results soon to be released). KKMR-03

24 24

25 25 KHRYSTHAL-2010

26 26

27 27

28 28 ( Alice is installing counters )

29 29

30 30 (And the same for Alice)

31 31 , KK,, New STAR@RHIC results on CEP with tagged forward protons soon to come. Prospects of CDP studies at ALICE & LHCb (Rainer)

32 32 Thank You  

33 33

34 34 UNCERTAINTIES Known Unknowns Unknown Unknowns N(N)LO- radiative effects (K-factors etc..) ‘…possible inadequancy of PT theory in  s …’ R.Barbieri et al-1980 ‘ ‘Right’ choice of gluon densities, in particular at so low scales as in the case ( potentiality of a factor of ~3 rise for the H-case ). Complete model for calculation of enhanced absorption. -experimental widths, decays… Gluons at so low scales, surprises are not excluded at all. Non- pQCD effects in the meson characteristics. Currently no complete description of heavy quarkonium characteristics. ‘ Two gluon width does not tell the whole story.’ Factor of 5 up or down (conservatively) Factor of 5 up or down (conservatively)

35 35

36 36 JINST-09

37 37

38 38


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