nonlinear evolution for pomeron fields in the semi classical

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Nonlinear evolution for Pomeron fields in the semi classical C. Contreras , E. Levin J. Miller* and R. Meneses Departamento de Física - Matemática Universidad Técnica Federico Santa María Valparaiso Chile *Lisboa Portugal SILAFAE 2012 Sao Paulo Brasil

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Nonlinear evolution for Pomeron fields in the semi classical. C. Contreras , E. Levin J. Miller* and R. Meneses Departamento de Física - Matemática Universidad Técnica Federico Santa María Valparaiso Chile *Lisboa Portugal SILAFAE 2012 Sao Paulo Brasil. O utlook. - PowerPoint PPT Presentation

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Page 1: Nonlinear evolution for  Pomeron fields in the semi classical

Nonlinear evolution for Pomeron fields

in the semi classical

C. Contreras , E. Levin J. Miller* and R. MenesesDepartamento de Física - Matemática

Universidad Técnica Federico Santa MaríaValparaiso Chile*Lisboa Portugal

SILAFAE 2012 Sao Paulo Brasil

Page 2: Nonlinear evolution for  Pomeron fields in the semi classical

OutlookIntroductionBFKL Pomeron Calculus and RFTSemi classical approximationSolution inside the saturation

regionApplication and Conclusion

Page 3: Nonlinear evolution for  Pomeron fields in the semi classical

IntroductionHigh Energy Scattering

Difractive Scattering and DIS : Pomeron exchange

h-h h-Nucleus Collision:dilute/dilute - dense sistema Nucleus - Nucleus CollisionDense-Dense systems

Page 4: Nonlinear evolution for  Pomeron fields in the semi classical

Scattering approachd=2 tranverse space

saturación region Qs >> C are

small then we can consider that semiclasicas approach are valid

Page 5: Nonlinear evolution for  Pomeron fields in the semi classical

Description in QCDThe interaction between particles is via

interchange of Gluons:

Color Singlet BFKL Pomeron Balinsky-Fadin-Kuraev-Lipatov

The amplitude can be described considering a Pomeron Green Function BFKL propagator

See Lipatov “ Perturbative QCD”

Page 6: Nonlinear evolution for  Pomeron fields in the semi classical

Where Dipole the wave function hep-th/0110325 Approximation r, R << b then it is

independent of b impact parameter

Page 7: Nonlinear evolution for  Pomeron fields in the semi classical

Balitsky-Fadin-Kuraev-Lipatov BFKL equation describe scattering amplitud in High Energy using a resumation LLA in pQCD (76-78)

BFKL evolution equation with respect to ln x , which are represented by a set of Gluon ladders

Intuitive Physical Picture: BFKL difussion in the IR region:

gluon radiation g -> gg in the transverse momentum kt exist large number of gluons but for small kt and large size of gluon and strongy overlap fusion gg –> g are important

Saturation phenomena

Page 8: Nonlinear evolution for  Pomeron fields in the semi classical

Experimental evidence in small-x

Page 9: Nonlinear evolution for  Pomeron fields in the semi classical
Page 10: Nonlinear evolution for  Pomeron fields in the semi classical
Page 11: Nonlinear evolution for  Pomeron fields in the semi classical
Page 12: Nonlinear evolution for  Pomeron fields in the semi classical
Page 13: Nonlinear evolution for  Pomeron fields in the semi classical
Page 14: Nonlinear evolution for  Pomeron fields in the semi classical

Approch to saturationFirst: Modification of the BFKL

1983 GLR Gribov, Levin and Ryskin

1999 BK Balisky- Kovchegov:include quadratic terms determined by three Pomeron VertexBK eq. evolution for Amplitude N(r,b,Y)

Page 15: Nonlinear evolution for  Pomeron fields in the semi classical

See hep.ph 0110325

BK equation DIS virtual photon on a large nucleus

LLA

Dipole approximation: photon splits in long before the interaction with nucleus degrees of freedoms

The dipole interacts independently with nucleons in the nucleus via two-gluon exchange

Page 16: Nonlinear evolution for  Pomeron fields in the semi classical
Page 17: Nonlinear evolution for  Pomeron fields in the semi classical

Approch to saturation IIColor Glass Condensate CGC Clasiccal field for QCD with Weizsacker-Williams generalized FieldMuller and Venogapalan

JIMWLK / KLWMIJ Equation J. Jalilian-Marian, E. Iancu, Mc Lerran, H. Weiger, A. Leonidovt and A. Kovner Renormalization Group Approach in the Y-variable

Page 18: Nonlinear evolution for  Pomeron fields in the semi classical

Generalization to Pomerones Interaction

1P 2P 2P 1PLoop de Pomerones

Page 19: Nonlinear evolution for  Pomeron fields in the semi classical

Pomeron Loops: See E. Levin, J. Miller and A Prygarin arXiv 07062944

For example: See Quantum Chromodynamic at High Eneregy Y. Kovchegov and E. Levin Cambridg 2011

BK resums the fan diagrams with the BFKL ladders Pomeron splitting into two ladders (GLR-DLA)

Loops of Pomeron are suppresed by power of A atomic number of the nucleus A

Page 20: Nonlinear evolution for  Pomeron fields in the semi classical

QCD results and effective action

Green Function

Definition of a Field Theory RFTSee M. Braun or E. Levin

Page 21: Nonlinear evolution for  Pomeron fields in the semi classical

Funcional Integral Braun ´00-06

Page 22: Nonlinear evolution for  Pomeron fields in the semi classical

Interaction with nucleus target / projectile

Page 23: Nonlinear evolution for  Pomeron fields in the semi classical

Solutions: momentum

representation

Page 24: Nonlinear evolution for  Pomeron fields in the semi classical

Equations and definitions

This equation is equivalent to: - BFKL if - BK

Page 25: Nonlinear evolution for  Pomeron fields in the semi classical

Semiclasical Approach

Page 26: Nonlinear evolution for  Pomeron fields in the semi classical

equations

Solution: Characteristica method

Page 27: Nonlinear evolution for  Pomeron fields in the semi classical

Using the relation BFKL PomeronL. Gribov, E. Levin and G. Ryskin Phy. Rep. 100 `83

One can show that

And that

Page 28: Nonlinear evolution for  Pomeron fields in the semi classical

We introduce

And we use de condition

Page 29: Nonlinear evolution for  Pomeron fields in the semi classical
Page 30: Nonlinear evolution for  Pomeron fields in the semi classical

Solution

Page 31: Nonlinear evolution for  Pomeron fields in the semi classical

Numerical SolutionExpanding around 𝛾→0

Page 32: Nonlinear evolution for  Pomeron fields in the semi classical

ConclusionPhysical Condition to select solutionExtension to Y dependenceAplication to Scattering dilute-Dense NucleusApplications: Scattering amplitudeIn a more refined analysis the b

dependence should be taken into accountRunning coupling effects sensitivity to IR

region and landau Pole!Solution in another regions

Page 33: Nonlinear evolution for  Pomeron fields in the semi classical

Preliminary Result

Page 34: Nonlinear evolution for  Pomeron fields in the semi classical

Kinematic VariablesQ resolution PowerX measure of momentum

fraction of struck quarkF(x,Q)

Page 35: Nonlinear evolution for  Pomeron fields in the semi classical

General BehaviourBjorken Limites DGLAP

Regge Limite