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      Nonlinear Gluon Evolution in the Color Glass Condensate: I

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          Abstract

          We consider a nonlinear evolution equation recently proposed to describe the small-\(x\) hadronic physics in the regime of very high gluon density. This is a functional Fokker-Planck equation in terms of a classical random color source, which represents the color charge density of the partons with large \(x\). In the saturation regime of interest, the coefficients of this equation must be known to all orders in the source strength. In this first paper of a series of two, we carefully derive the evolution equation, via a matching between classical and quantum correlations, and set up the framework for the exact background source calculation of its coefficients. We address and clarify many of the subtleties and ambiguities which have plagued past attempts at an explicit construction of this equation. We also introduce the physical interpretation of the saturation regime at small \(x\) as a Color Glass Condensate. In the second paper we shall evaluate the expressions derived here, and compare them to known results in various limits.

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          Green's Functions in the Color Field of a Large Nucleus

          We compute the Green's functions for scalars, fermions and vectors in the color field associated with the infinite momentum frame wavefunction of a large nucleus. Expectation values of this wavefunction can be computed by integrating over random orientations of the valence quark charge density. This relates the Green's functions to correlation functions of a two dimensional, ultraviolet finite, field theory. We show how one can compute the sea quark distribution functions, and explictly compute them in the kinematic range of transverse momenta, \(\alpha_s^2 \mu^2 << k_t^2 << \mu^2\), where \(\mu^2\) is the average color charge squared per unit area. When \(m_{quark}^2 << \mu^2 \sim A^{1/3}\), the sea quark contribution to the infinite momentum frame wave function saturates at a value that is the same as that for massless sea quarks.
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            Gluon Production from Non-Abelian Weizs\"acker-Williams Fields in Nucleus-Nucleus Collisions

            We consider the collisions of large nuclei using the theory of McLerran and Venugopalan. The two nuclei are ultra-relativistic and sources of non-abelian Weizs\"acker-Williams fields. These sources are in the end averaged over all color orientations locally with a Gaussian weight. We show that there is a solution of the equations of motion for the two nucleus scattering problem where the fields are time and rapidity independent before the collision. After the collision the solution depends on proper time, but is independent of rapidity. We show how to extract the produced gluons from the classical evolution of the fields.
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              Relating different approaches to nonlinear QCD evolution at finite gluon density

              We analyze the relation between evolution equations at low x that have been derived in different approaches in the last several years. We show that the equation derived by Balitsky and Kovchegov is obtained from the Jalilian-Marian-Kovner-Leonidov-Weigert (JKLW) equation in the limit of small induced charge density. We argue that the higher nonlinearities resummed by the JKLW equation correspond, in physical terms, to the breakdown of the eikonal approximation when the gluon fields in the target are large.
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                Author and article information

                Journal
                20 November 2000
                Article
                10.1016/S0375-9474(01)00642-X
                hep-ph/0011241
                f2fab1de-76f4-4ac0-be3a-413644b8128c
                History
                Custom metadata
                Saclay-T00/166, BNL-NT-00/24
                Nucl.Phys. A692 (2001) 583-645
                67 pages, 7 eps figures
                hep-ph

                High energy & Particle physics
                High energy & Particle physics

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