1 / 57

Why GLR-MQ-ZRS equation is necessary for understanding STAR BES program?

Wei Zhu East China Normal University KITPC  20 12 . 07. Why GLR-MQ-ZRS equation is necessary for understanding STAR BES program?. Nuclear suppression factor. Unintegrated distribution=TMD. =TMD. Reasons. 1. Integrated and unintegrated gluon distributions can not directly

ayame
Download Presentation

Why GLR-MQ-ZRS equation is necessary for understanding STAR BES program?

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Wei Zhu East China Normal University KITPC 2012.07. Why GLR-MQ-ZRS equation is necessary for understanding STAR BES program?

  2. Nuclear suppression factor

  3. Unintegrated distribution=TMD =TMD

  4. Reasons 1. Integrated and unintegrated gluon distributions can not directly measured, they only can been extracted from data using QCD evolution equations. 2. 3. We need a QCD evolution equation, which includes nuclear shadowing and antishadowing effects.

  5. Why not? • DGLAP Equation. Nuclear shadowing and antishadowing effects are assumed in input by hand.

  6. Why not • BFKL equation, It works at x< and has not nonlinear corrections. • BK equation=BFKL+gluon fusion. It works at x< and does not consider the antishadowing corrections. • .

  7. JIMWLK equation • Although it predicts the saturation at small x limit, however, can not describe the parton distributions at < x<1.

  8. Only GLR-MQ-ZRS Equation1983 version • L.V. Gribov, E.M. Levin and M.G. Ryskin, Phys. Rep.100 (1983) 1.

  9. Fusion Corrections of Gluon Fusion DGLAP DGLAP GLR-MQ-ZRS to 3

  10. Abramovsky, Gribov and Kancheli, Cutting rule (1973) 1 -4 2

  11. 1986 version • A.H. Mueller and J. Qiu, Nucl. Phys. B268 (1986) 427.

  12. W. Zhu, Nucl. Phys. B551 (1999) 245. W. Zhu and J.H.Ruan, Nucl. Phys. B559 (1999) 378; W. Zhu and Z.Q. Shen, HEP$\&$ NP, 29 (2005) 109. 1999 version

  13. ZRS versionTOPT cutting rule

  14. TOPT Cutting Rules • F.E. Close, J. Qiu and R.G. Roberts, Phys. Rev. D 40 (1989) 2820. • W. Zhu, Nucl. Phys. B551, 245 (1999). • W. Zhu and J.H. Ruan, Nucl. Phys. B559, 378(1999). • W. Zhu, Z.Q. Shen and J.H. Ruan, Nucl. Phys. B692, 417 (2004);

  15. TOPT-Cutting rule • List all possible TOPT diagrams with different cuts. • The contributions of the cut diagrams • have the identical integral kernel with only the following different factors R:

  16. (a)The sign in the first factor is determined by the energy deficits; • (b)The second factor takes a value of 1/2 if the probe-vertex inserts in the initial line; • (c) function relates to the probe vertex.

  17. Recombination functions

  18. 4. Twist-4 level (collinear frame) CVPT generalize Mueller-Qiu (1986) to whole x region

  19. TOPT:Zhu, Ruan (1999); Bluemlein, Ravindran, Ruan, Zhu (2001); Zhu,Shen (2004)

  20. Spin-dependent gluon recombination function

  21. Why yes? • GLR-MQ-ZRS equation has solid QCD basic. • LL(Q^2). 0.001<x<1. • DLL(1/x,Q^2). 0.001<0.1-0.2

  22. GLR-MQ-ZRS at small x

  23. Cronin Effect

  24. Nuclear modification factor

  25. KMR Scheme

  26. Nuclear shadowing and antishadowing effects • A+A(for gluon)>p+A(for gluon) • ~eA(for gluon)>eA(for quarks) • Contributions of the gluon fusion at initial state are inescapable in RHIC and LHC physics.

  27. ?

  28. ? ???

  29. arXiv:1012.4224W. Zhu, J.H. Ruan and F.Y. Hou • A rapid crossover from week energy • loss to strong energy loss at a universal critical energy of gluon jet Ec ∼ 10GeV

More Related