Acessibilidade / Reportar erro

BK equation and traveling wave solutions

Abstract

It has been shown that the transition to the saturation regime of high energy QCD is similar to the formation of the front of a traveling wave. In particular, it can be verified that Balitsky-Kovchegov (BK) evolution equation reduces, after some approximations, to the nonlinear Fisher and Kolmogorov-Petrovsky-Piscounov (FKPP) equation, well-known from statistical physics. In these proceedings, based on the current knowledge of the asymptotic solutions of the BK equation, we propose a parametrization for the forward scattering amplitude which interpolates between the traveling wave solution and the saturation region.

Traveling waves; Transition to saturation


POSTERS

BK equation and traveling wave solutions

J. T. de Santana AmaralI; M. A. BetempsI; M. B. Gay DucatiI; G. SoyezI, * * On leave from the fundamental theoretical physics group of the University of Liège

IInstituto de Física, Universidade Federal do Rio Grande do Sul, 91501 Porto Alegre (RS), Brazil

IIService de Physique Theorique de Saclay, CEA/DSM/SPhT, F-91191 Gif-sur-Yvette, France

ABSTRACT

It has been shown that the transition to the saturation regime of high energy QCD is similar to the formation of the front of a traveling wave. In particular, it can be verified that Balitsky-Kovchegov (BK) evolution equation reduces, after some approximations, to the nonlinear Fisher and Kolmogorov-Petrovsky-Piscounov (FKPP) equation, well-known from statistical physics. In these proceedings, based on the current knowledge of the asymptotic solutions of the BK equation, we propose a parametrization for the forward scattering amplitude which interpolates between the traveling wave solution and the saturation region.

Keywords: Traveling waves; Transition to saturation

I. INTRODUCTION

Solving the problem of the growth of the cross sections for hadronic interactions with energy is still an important challenge in Quantum Chromodynamics (QCD). As well-known, the increase of energy causes a fast growth of the gluon density and consequently of the cross sections. At very high energies, it is expected that, at some point, gluon recombination and multiple scattering might be important and unitarity can be restored. This phenomenon is called saturation and has been deeply investigated over the last thirty years [1-6].

From the theoretical side, the main contribution to describe and understand the saturation in high energy QCD comes from the development of non-linear QCD equations describing the evolution of scattering amplitudes towards this limit. The simplest of such equations is the Balitsky-Kovchegov (BK) equation [7, 8], which corresponds to the Balitsky-Fadin-Kuraev-Lipatov (BFKL) [9] linear evolution equation with the addition of a non-linear term responsible for the tame of the growth of gluon density.

From the phenomenological side one has the discovery of geometric scaling in deep inelastic scattering (DIS) at HERA [10]. This phenomenological feature of high energy DIS is expressed as a scaling property of the virtual photon-proton cross section

that is, the cross section depends on the scaling variable t = Q2/(Y) instead of Q2 and (Y) separately. Here Q is the virtuality of the photon, Y is the total rapidity (Y = log(1/x)) and Qs(Y) is an increasing function of Y called saturation scale. Indeed, geometric scaling has a natural explanation [11] in terms of traveling wave solutions of the BK equation.

In these proceedings we use the dipole model [12] to relate the g*p cross section to the dipole-proton forward scattering amplitude through a parametrization for the latter in momentum space. In Section II we relate to the dipole-proton scattering amplitude through the dipole framework. In Section III we introduce the BK equation which describes the dipole scattering amplitude and the properties of its solutions, and from these we build the parametrization for the amplitude in Section IV. In Section V we present the conclusions and discuss the applications of our model.

II. MUELLER'S DIPOLE PICTURE

Let us consider the collision between a virtual photon and a proton at high energy. In a frame where the photon travels fast, but most of the energy is still carried by the proton, one can consider that the photon fluctuates into a (quark-antiquark) pair, a colorless dipole, which then interacts with the proton [12]. In the leading logarithmic approximation (LLA) of perturbative QCD (pQCD), the cross section factorizes and one gets the well-known formula

where r is the size of the dipole, z is the longitudinal momentum fraction of the photon carried by the quark and (r,Y) is the dipole-proton cross section. Assuming an independence on the impact parameter of the collision, this cross section is proportional to the proton-dipole forward scattering amplitude, T(r,Y), through the relation

where is the proton radius. As we shall see in the next section, the amplitude T(r,Y) obeys the BK equation in coordinate space but the asymptotic behaviour of its solutions is naturally expressed in momentum space. We want to express in terms of (k,Y), the Fourier transform of T(r,Y):

III. SCATTERING AMPLITUDES AT HIGH-ENERGY

Consider now a fast-moving colorless dipole of transverse size r = |x-y|, where x and y are the coordinates of the quark and antiquark, respectively, interacting with a given dense target. In the large-Nc approximation (Nc is the number of colors), and in the mean-field approximation, the high-energy behaviour of the dipole forward scattering amplitude T(x,y;Y) follows the BK equation [7, 8]. In coordinate space this equation reads

which, as it was said in the Introduction, corresponds to the BFKL equation (the first three terms inside the brackets), but with an additional term (the term quadratic in T) which by its turn corresponds to the nonlinear effects responsible for the decreasing of the growth in the gluon density. Here = as Nc/p, as is the strong coupling constant (considered fixed). If one neglects the dependence on the impact parameter b = (x+y)/2 and integrates out the remaining angular dependence of r, Eq.(4) becomes an equation for T(r,Y). The latter can be expressed in momentum space through (3).

The amplitude (k,Y) obeys the BK equation in momentum space

where as is the strong coupling constant, Nc is the number of colours,

is the characteristic function of the Balitsky-Fadin-Kuraev-Lipatov (BFKL) kernel [9] and

where k0 is some fixed low momentum scale. The kernel c(g) is an integro-differential operator which may be defined with the help of the formal series expansion

for some g0 between 0 and 1, i.e. for the principal branch of the function c.

A. Traveling wave solutions

If one performs the following change of variables

it has been shown [11] that the BK equation reduces to the Fisher and Kolmogorov-Petrovsky-Piscounov (F-KPP) equation [13] for u when its kernel (6) is approximated by the first three terms of the expansion, the so-called diffusive approximation. The F-KPP equation is a well-known equation in non-equilibrium statistical physics, whose dynamics is called reaction-diffusion dynamics, and it has the form

where t is time and x is the coordinate. This equation admits the so-called traveling wave solutions.

For a traveling wave solution one can define the position of a wave front x(t) = v(t), irrespective of the details of the nonlinear effects. At larger times, the shape of a traveling wave is preserved during its propagation, and the solution becomes only a function of the scaling variable x - vct, where vc is the critical velocity.

In the language of saturation physics the position of the wave front is nothing but the saturation scale

and the scaling cited above corresponds to the geometric scaling

The linear part of (5) is solved by [11]

where

0(g) is the Mellin transform of the initial condition at Y = 0. The velocity of the front is given by

where gc is the saddle point of the exponential phase factor. This fixes, for the BFKL kernel, gc = 0.6275..., and vc = 4.88.

In terms of QCD variables, the dipole forward scattering amplitude in momentum space in the tail of the wave front reads

The saturation scale is defined as

IV. CONNECTION WITH SATURATION

The goal of this work is to describe the matching around the saturation scale between two regions: the one described by the tail of the wave front, Eq.(13) and the other one, characterized by saturation. The latter can be parametrized as

where c is an arbitrary constant.

Given that the fully asymptotic behaviour of the amplitude is described by (14) and (16), our first attempt to connect both was to use both behaviours separately and match the constant c from continuity conditions (see Figure 4).


However, such matching procedure does not necessarily imply a positive Fourier transform of the scattering amplitude. Then, the best way to obtain the description of such transition to the saturation region is to make an analytic interpolation procedure. The idea is to build the saturation domain from the dilute one and the starting point is a function, that we call

dil, which reproduces (up to the logarithmic factor) the amplitude for diffusive scaling (14),

with

and write in terms of it in such a way that we can recover the asymptotic behaviours of , i.e., Eqs. (14) and (16).

One expression which satisfies these properties is the following:

where the logarithmic factor

The constants A and K can be determined by applying the parametrization proposed to describe some physical observable, for example, via fitting procedure to some experimental data. Such procedure could be a good way to test the robustness of our model.

V. CONCLUSIONS

In this work we have investigated the matching between saturation and travelling wave solutions of the BK equation which describe the forward scattering amplitude at high energies in the virtual photon-proton scattering. As the result does not necessarily imply a positive Fourier transform of the amplitude, we concluded that the best way to connect both solutions is through an analytic interpolation model. An expression for the amplitude, Eqs.(17)-(20), has been proposed and tested in order to be used to describe some experimental data. This work is in progress.

Acknowledgements

This work is partially supported by CNPq, Brazil. G.S. is funded by the National Funds for Scientific Research (FNRS, Belgium).

[1] L. V. Gribov, E. M. Levin, and M. G. Ryskin, Phys. Rep. 100, 1 (1983).

[2] A. H. Mueller and J. Qiu, Nucl. Phys. B 268, 427 (1986).

[3] A. H. Mueller, Nucl. Phys. B 335, 115 (1990).

[4] J. Jalilian-Marian, A. Kovner, A. Leonidov, and H. Weigert, Nucl. Phys. B 504, 415 (1997) [ arXiv:hep-ph/9701284]; E. Iancu, A. Leonidov, and L. D. McLerran, Nucl. Phys. A 692, 583 (2001) [ arXiv:hep-ph/0011241]; H. Weigert, Nucl. Phys. A 703, 823 (2002) [ arXiv:hep-ph/0004044].

[5] A. L. Ayala, M. B. Gay Ducati, and E. M. Levin, Nucl. Phys. B 493, 305 (1997); Nucl. Phys. B 551, 335 (1998).

[6] Yu. V. Kovchegov and A. H. Mueller, Nucl. Phys. B 529, 451 (1998).

[7] I. I. Balitsky, Nucl. Phys. B 463, 99 (1996); Phys. Rev. Lett. 81, 2024 (1998); Phys. Lett. B 518, 235 (2001); arXiv:hep-ph/0101042.

[8] Y. V. Kovchegov, Phys. Rev. D 60, 034008 (1999); 61, 074018 (2000).

[9] L. N. Lipatov, Sov. J. Nucl. Phys. 23, 338 (1976); E. A. Kuraev, L. N. Lipatov, and V. S. Fadin, Sov. Phys. JETP 45, 199 (1977); I. I. Balitsky and L. N. Lipatov, Sov. J. Nucl. Phys. 28, 822 (1978).

[10] A. M. Stasto, K. Golec-Bernat, and J. Kwiecinski, Phys. Rev. Lett. 86, 596 (2001).

[11] S. Munier and R. Peschanski, Phys. Rev. Lett. 91, 232001 (2003); Phys. Rev. D 69, 034008 (2004); Phys. Rev. D 70, 077503 (2004).

[12] A. H. Mueller, Nucl. Phys. B 415, 373 (1994); A. H. Mueller and B. Patel, Nucl. Phys. B 425, 471 (1994); A. H. Mueller, Nucl. Phys. B 437, 107 (1995).

[13] R. A. Fisher, Ann. Eugenics 7, 355 (1937); A. Kolmogorov, I. Petrovsky, and N. Piscounov, Moscou Univ. Bull. Math. A 1, 1 (1937).

Received on 1st December, 2006

  • [1] L. V. Gribov, E. M. Levin, and M. G. Ryskin, Phys. Rep. 100, 1 (1983).
  • [2] A. H. Mueller and J. Qiu, Nucl. Phys. B 268, 427 (1986).
  • [3] A. H. Mueller, Nucl. Phys. B 335, 115 (1990).
  • [4] J. Jalilian-Marian, A. Kovner, A. Leonidov, and H. Weigert, Nucl. Phys. B 504, 415 (1997) [
  • arXiv:hep-ph/9701284]; E. Iancu, A. Leonidov, and L. D. McLerran, Nucl. Phys. A 692, 583 (2001) [
  • arXiv:hep-ph/0011241]; H. Weigert, Nucl. Phys. A 703, 823 (2002) [
  • [5] A. L. Ayala, M. B. Gay Ducati, and E. M. Levin, Nucl. Phys. B 493, 305 (1997);
  • Nucl. Phys. B 551, 335 (1998).
  • [6] Yu. V. Kovchegov and A. H. Mueller, Nucl. Phys. B 529, 451 (1998).
  • [7] I. I. Balitsky, Nucl. Phys. B 463, 99 (1996);
  • Phys. Rev. Lett. 81, 2024 (1998);
  • Phys. Lett. B 518, 235 (2001);
  • [8] Y. V. Kovchegov, Phys. Rev. D 60, 034008 (1999); 61, 074018 (2000).
  • [9] L. N. Lipatov, Sov. J. Nucl. Phys. 23, 338 (1976);
  • E. A. Kuraev, L. N. Lipatov, and V. S. Fadin, Sov. Phys. JETP 45, 199 (1977);
  • I. I. Balitsky and L. N. Lipatov, Sov. J. Nucl. Phys. 28, 822 (1978).
  • [10] A. M. Stasto, K. Golec-Bernat, and J. Kwiecinski, Phys. Rev. Lett. 86, 596 (2001).
  • [11] S. Munier and R. Peschanski, Phys. Rev. Lett. 91, 232001 (2003);
  • Phys. Rev. D 69, 034008 (2004);
  • Phys. Rev. D 70, 077503 (2004).
  • [12] A. H. Mueller, Nucl. Phys. B 415, 373 (1994);
  • A. H. Mueller and B. Patel, Nucl. Phys. B 425, 471 (1994);
  • A. H. Mueller, Nucl. Phys. B 437, 107 (1995).
  • [13] R. A. Fisher, Ann. Eugenics 7, 355 (1937);
  • A. Kolmogorov, I. Petrovsky, and N. Piscounov, Moscou Univ. Bull. Math. A 1, 1 (1937).
  • *
    On leave from the fundamental theoretical physics group of the University of Liège
  • Publication Dates

    • Publication in this collection
      13 Aug 2007
    • Date of issue
      July 2007

    History

    • Received
      01 Dec 2006
    Sociedade Brasileira de Física Caixa Postal 66328, 05315-970 São Paulo SP - Brazil, Tel.: +55 11 3091-6922, Fax: (55 11) 3816-2063 - São Paulo - SP - Brazil
    E-mail: sbfisica@sbfisica.org.br