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Exclusive charmonium production in hard exclusive processes. V.V. Braguta Institute for High Energy Physics Protvino, Russia
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Content: Introduction Charmonium Distribution Amplitudes (DA) The properties of DAs Exclusive charmonium production within light cone formalism: Perspectives
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Introduction
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Internal structure of charmonium First approximation Charmonium = nonrelativistic quark-antiquark bound state Charmonium spectrum Next approximation: NRQCD Charmonium = nonrelativistic system v 2 ~0.3, v~0.5 Production as a probe of the internal structure of charmonium
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NRQCD formalism At LO of NRQCD quark-antiquark pair has zero relative momentum
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Light Cone Formalism The amplitude is divided into two parts:Hadronization Twist-2 2-distribution amplitudes Twist-3 4-distribution amplitudes … … Light cone formalism is designed to study hard exclusive processes
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Comparison of LCF and NRQCD The cross section is double series LCF Power corrections: NRQCD Relativisitic corrections: Radiative corrections:
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Relativistic corrections LCFNRQCD DA resums relativististic corrections to the amplitude.
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Leading logarithmic radiative corrections Exclusive quarkonium production Inclusive quarkonium production DA resums leading logarithmic radiative corrections.
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Distribution Amplitudes are the key ingredient of Light Cone Formalism
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Charmonium Distribution Amplitudes
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Definitions of leading twist DA
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Evolution of DA DA can be parameterized through the coefficients of conformal expansion a n : Alternative parameterization through the moments:
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DA of nonrelativistic system
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Different approaches to the study of DA 1. Functional approach - Bethe-Salpeter equation 2. Operator approach - NRQCD - QCD sum rules
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Potential models Solve Schrodinger equation Get wave function in momentum space: Make the substitution in the wave function: Integrate over transverse momentum: Brodsky-Huang-Lepage procedure:
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Different approaches
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The moments within Potential Models The larger the moment, the larger the contribution of relativistic motion Only few moment can be calculated Higher moments contain information about relativistic motion in quarkonium
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Is there relativistic motion in quarkonium? Relativistic motion can appear only due to the rescatering for a short period of time (v<<1) Relativistic motion exists v 2 ~0.3 is still large
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Property of DA DA of nS state has 2n+1 extremums
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The moments within NRQCD
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The values of were calculated in paper G. Bodwin, Phys.Rev.D74:014014,206 The constant can be expressed through the
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The model for DA within NRQCD At leading order approximation is the only parameter
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The moments of DA within QCD sum rules Advantage: The results are free from the uncertainty due to the relativistic corrections Disadvantage: The results are sensitive to the uncertainties in the sum rules parameters: QCD sum rules is the most accurate approach
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The details of the calculation
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Logitudinally polarized 3 S 1 mesons Sum rules Improved Sum rules: Sum rules parameters:
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Numerical analysis
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The other DAs These sum rules are less accurate
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The results of the calculation The results for 1S states The results for 2S states
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The models of DAs 1S states 2S states Borel version sum rules without vacuum condensates
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The properties of distribution amplitudes
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Relativistic tail At DA is suppressed in the region Fine tuning is broken at due to evolution This suppression can be achieved if there is fine tuning of a n
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Relativistic tail within NRQCD Light Cone The amplitude of meson production NRQCD Leading logarithmic corrections are resummed in DA Leading logarithmic corrections are contained in Wilson coefficients QCD radiative corrections enhance the role of higher NRQCD operators
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The violation of NRQCD scaling rules At larger scales the fine tuning of the coefficients a n is broken and NRQCD scaling rules are violated NRQCD velocity scaling rules are violated in hard processes
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Improvement of the model for DA The evolution of the second moment The accuracy of the model for DA is better at larger scales
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Models for 2S states At leading order approximation of NRQCD the relative momentum of quark-antiquark pair is zero
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Exclusive charmonium production within light cone formalism
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The processes:
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The diagrams Fragmentation diagrams Nonfragmentation diagrams
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The cross section at NLO
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Relativistic and leading logarithmic radiative corrections Interference of fragmentation and nonfragmentation diagrams The role of corrections
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The results of the calculation a Bodwin, Braaten, Lee, Phys. Rev. D74
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The processes:
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e + e - V( 3 S 1 ) P( 1 S 0 ) This formula was first derived in Bondar, Chernyak, Phys. Lett. B612, 215 (2005)
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Twist-3 distribution amplitudes are unknown Problem: The scale dependences of some twist-3 DAs are unknown
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The constants needed in the calculation The values of the constants The values of the constants (preliminary results)
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The results of the calculation Why LO NRQCD is much smaller than the experimental results? 1. Relativistic corrections K~2.5-6 2. Leading logarithmic radiative corrections K~1.5-2.5 a E. Braaten, J. Lee b K.Y. Liu, Z.G. He, K.T. Chao
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Relativistic and radiative corrections NRQCD formalism Light cone formalism The amplitude was derived in paper Bondar, Chernyak, Phys.Lett. B612
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Perspectives: Theoretical LCF can resolve the other problems with exclusive processes? Development of alternative to NRQCD DAs of P-wave and D-wave charmonium mesons New results for bottomonium decays Inclusive charmonium production Experimental LHC (bottomonium decays) B-factories and Super B-factories (exclusive production of mesons and baryons)
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