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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 Quarkonia. (KHRYSTHAL collaboration)

V.A. Khoze ( IPPP, Durham )

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Central Diffractive Production of Heavy Quarkonia. (KHRYSTHAL collaboration). . V.A. Khoze ( IPPP, Durham ). (based on works by V. KH oze, M. RY sk in and W.J. ST irling and L. HA rland -L ang ). 1. With a bit of personal flavour. (topical examples ). Tevatron, RHIC and LHC. - PowerPoint PPT Presentation

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Page 1: V.A. Khoze ( IPPP, Durham )

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V.A. Khoze (IPPP, Durham)

(based on works by V.KHoze, M. RYskin and W.J. STirling and L. HArland-Lang)

Central Diffractive Production ofHeavy Quarkonia.

(KHRYSTHAL collaboration)

Page 2: V.A. Khoze ( IPPP, Durham )

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Forward proton distributions and correlations.

Tevatron, RHIC and LHC.

CDP@LHC with FSC

(topical examples)With a bit of personal flavour

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(star reactions!)

New D0 jj- resultsRHIC, ALICE data expected

Detailed tests of dynamics of soft diffraction (KMR-02)

Spin-Parity Analyzer (KKMR-2003)

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,b

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• 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

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“soft” scattering can easily destroy the gaps

gap

gap

eikonal rescatt: between protonsenhanced rescatt: involving intermediate partons

M

soft-hardfactorizn

conservedbroken

Subject of hot discussions recently :Subject of hot discussions recently : S²S²enhenh

S² absorption effects -necessitated by unitarity

Everybody’s ~ happy (KMR, GLMM, FHSW, KP, S.Ostapchenco. Petrov et al, BH, GGPS, MCs..)

(Beatriz)

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‘Better to light a candle than to rant against darkness’

( Confucius )

Standard Candle ProcessesStandard Candle Processes

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Our 3 measurements are all in good agreement (factor “few”) with the Durham group predictions.

*

*

*Prpospects !

FSC@LHC

(more coming soon )

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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

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(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

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1111

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Charmonium –like XYZ states

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still unobserved

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

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What we expect within the framework of the Perturbative Durham formalism (KMR-01, KKMR-03, KMRS-04, HKRS-10)

Example, O++ -case

*KNLO

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

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Too good to be true ?!

Phys.Rev.Lett.102:242001,2009

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(HKRS-09,10)

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(A. Alekseev-1958-positronium)

(R.Pasechnik et al, Phys.Lett.B680:62-71,2009; HKRS, Eur.Phys.J.C65:433-448,2010)

KMR-01

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1 : 0.6 : 0.22

2

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20Spin-parity Analyzer

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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 % .

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1 : 0.03 : 0.08

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(0 ) /d d

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

KKMR-03

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KHRYSTHAL-2010

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( Alice is installing counters )

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(And the same for Alice)

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, KK, ,

New STAR@RHIC results on CEP with tagged forward protons soon to come.

Prospects of CDP studies at ALICE & LHCb (Rainer)

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Thank You

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UNCERTAINTIES 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.

c

b

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 Factor of 5 up or down (conservatively) (conservatively)

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JINST-09

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