V.A. Khoze ( IPPP, Durham )
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Transcript of V.A. Khoze ( IPPP, Durham )
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V.A. Khoze (IPPP, Durham)
(In collaboration with L. Harland-Lang, M. Ryskin and W.J. Stirling)
Outlook on Central Diffractive Processes at the Tevaron , LHC and RHIC
CDP
07 May 2010, CERNDIFFRACTION@LH
C
7 May 2010
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Forward proton distributions and correlations.
Tevatron, LHC and RHIC.
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(star reactions!)
D0, RHIC datato come soon
Detailed tests of dynamics of soft diffraction (KMR-02)
Spin-Parity Analyzer
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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 nowadays :Subject of hot discussions nowadays : S²S²enhenh
S² absorption effects -necessitated by unitarity
Everybody’s ~ happy (KMR, GLMM, FHSW, KP,Petrov et al, BH, GGPS, Luna...MCs)
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‘Better to light a candle than to rant against darkness’
( Confucius )
Standard Candle ProcessesStandard Candle Processes
CDF & DO (Christina, Mike)
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7
(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
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Our 3 measurements are all in good agreement (factor “few”) with the Durham group predictions.
*
*
*Prpospects !
FSC@LHC (Mike)
(more coming soon )
(Christina, Mike)
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(Gap Detectors in no P-U events)
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What we expect within the framework of the 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
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)
Diphoton CEP
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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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and accounted for in the integrand
CDF
Spin-parity Analyzer
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Central Diffractive Production of
(Crystal Ball -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(HKRS results soon to come).
KKMR-03
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0+ 1+
2+ 0-
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0+ 1+
2+0-
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(HKRS-2010)
HKRS-results at different energies, and cuts are now available.
New(Leading term QCD expectations)
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Central production with RPs @STAR is taking of. First pppXp data.Partial wave analysis- soon.
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Rich diffractive structure of the cross sections as a function of proton momenta
Ongoing HKRS studies for RHIC energies and kinematics.Correlations between transverse momenta of outgoing protons
KMR-02
Interesting to compare the results for different states.
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LHCbExcellent particle ID (pion/Kaonseparation), vertex and proper
time resolutionexotic states….
Potentially rich program of CDP studies with the LHCb
JINST 4:P11019,2009.
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Disclaimer : up to the experts to deliver a verdict
JINST 4:P11019,2009.
(CDP background to the luminometer )
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, KK, ,
, dijet, diphton CEP- rich program of studies at the LHC; promising potential of LHCb.
New STAR@RHIC results on CEP with tagged forward protons soon to come.
Currently active studies are in progress (both in theory and experiment).
Prospects of CDP studies at ALICE (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 (at best) (at best)
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)
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and
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MRST99 and MSTW08LO PDFs provide approximately upper and lower bounds respectively
Ratios of cross sections at different energies- uncertainties
DIPHOTON CEP
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Are the early LHC runs,without proton taggers,able to check estimatesfor pp p+A+p ?
Possible checks of:
(i) survival factor S2: W+gaps, Z+gaps
(ii) generalised gluon fg : p p
(iii) Sudakov factor T : 3 central jets
(iv) soft-hard factorisation #(A+gap) evts (enhanced absorptive corrn) #(inclusive A) evts with A = W, dijet, …
gap
gapKMR: 0802.0177
Divid
e et
Impe
ra