Partonic transverse momenta in soft collisions

Open Access
Regular Article - Theoretical Physics

Abstract

The partonic transverse momentum, \(k_t\), distribution plays a crucial role in driving high-energy hadron interactions. If \(k_t\) is limited we have old fashioned Regge theory. If \(k_t\) increases with energy the interaction may be described by perturbative QCD. We use BFKL diffusion in \(\ln k_t\), supplemented by a stronger absorption of low \(k_t\) partons, to estimate the growth of the mean transverse momenta \(\langle k_t\rangle \) with energy. This growth reveals itself in the distribution of secondaries produced at the collider energies. We present a simple, BFKL-based, model to demonstrate the possible size of the effect. Moreover, we propose a way to evaluate experimentally the shape of the parton transverse momenta distribution by studying the spectra of the (\(D\) or \(B\)) mesons which contain one heavy quark.

Keywords

Transverse Momentum Heavy Quark Gluon Distribution Transverse Momentum Distribution Heavy Meson 

1 Introduction

Contrary to old Regge theory, where it was assumed that the transverse momenta of all the particles are limited, QCD is a logarithmic theory where there is a possibility that the parton’s (quark, gluon) transverse momentum may increase during the evolution. In particular, already in leading order (LO) BFKL evolution there is diffusion in \(\ln k_t\) space [1, 2]. From the experimental point of view, it is relevant to note that the growth of the mean transverse momenta, \(\langle p_t\rangle \), of secondary hadrons with collider energy was observed at the Tevatron and at the LHC (see e.g. [3, 4]). In order to describe this growth in DGLAP-based Monte Carlo generators [5, 6] an additional infrared cutoff, \(k_\mathrm{min}\), was introduced. Of course, in any case, we need a cutoff to avoid the infrared divergence of the amplitude of the hard (parton–parton interaction) subprocess. However, at first sight, we would expect this cutoff to have its origin in confinement. It should be less than 1 GeV and should not depend on energy. On the contrary, it turns out that to reproduce the energy dependence of the data, the value of \(k_\mathrm{min}\) should increase as \(k_\mathrm{min}\propto s^{0.12}\) [5]; such that at the Tevatron energy \(k_\mathrm{min}\simeq 2\) GeV, while at the LHC \(k_\mathrm{min}\simeq 3\) GeV.

In Sect. 2 we present a simple model which accounts for BFKL \(\ln k_t\) diffusion, together with the absorptive effects which additionally suppress the low \(k_t\) partons, since the absorptive cross section behaves as \(\sigma ^\mathrm{abs}\propto 1/k^2_t\). That is, we now have a dynamically induced infrared cutoff.1 In Sect. 3 we use this model to obtain the expected energy and rapidity dependence of \(k_t\) distributions. In Sect. 4, we discuss the possibility to directly study these effects experimentally by measuring the \(p_t\) spectra of \(D\) (and/or \(B\)) mesons. Due to the strong leading particle effect (see e.g. [11, 12, 13]) the transverse momentum of mesons which contain a heavy quark is close to the transverse momentum of the heavy quark. Moreover, final-state interactions and confinement do not appreciably distort the original distribution of these heavy mesons.

2 BFKL-based model

The original BFKL equation [14, 15, 16, 17] may be written as an integral equation for the gluon distribution unintegrated over \(k_t\),
$$\begin{aligned} f(x,k_t)=\partial [xg(x,k^2_t)]/\partial [d\ln k^2_t], \end{aligned}$$
(1)
in the form
$$\begin{aligned} f(x,k_t)&= f_0(x,k_t) + \frac{\alpha _s}{2\pi } \int _x^1 \frac{{\text {d}} z}{z} \int _{k_0}^\infty \frac{d^2k'_t}{\pi } \nonumber \\&\times \, \mathcal{K}(k_t,k'_t,z)~f(x/z,k'_t), \end{aligned}$$
(2)
where the kernel is evaluated as
$$\begin{aligned}&\mathcal{K}(k_t,k_t',z)f(x/z,k'_t)\nonumber \\&\quad = 2N_c\frac{k^2_t}{k^{'2}_t}\left[ \frac{f(x/z,k'_t)-f(x/z,k_t)}{|k^{'2}_t-k^2_t|} ~+~\frac{f(x/z,k_t)}{\sqrt{4k^{'4}_t+k^4_t}}\right] .\nonumber \\ \end{aligned}$$
(3)
The first term in the kernel2 can be understood as the effect of the emission of a daughter gluon with momentum (\(x,k_t\)) from a parent gluon with momentum (\(x'=x/z, k_t'\)). This generates the ladder structure of the pomeron sketched in Fig. 1a. The remaining two terms in the kernel (depending on \(f(x/z,k_t)\)) account for the loop corrections which occur in the trajectory of \(t\)-channel reggeised gluons.
Fig. 1

a BFKL ladder diagram; b the ladder structure of the triple-pomeron coupling

It is important to evolve in \(k_t\) (as well as \(x\)) to be able to understand the origin and the behaviour of the dynamical infrared cutoff—that is, to see how the \(k_t(s,y)\) distribution is generated within perturbative QCD. Here \(y= \ln (1/x)\) is the rapidity of the parton. This dynamically generated cutoff affects (i) the \(p_T\) distribution of secondary hadrons, (ii) the slope, \(\alpha '_P\), of the (QCD) pomeron trajectory and (iii) the values of the triple- and multi-pomeron couplings which control the predictions of the cross sections for diffractive dissociation.

Equation (2) can be solved numerically, starting, for example, from an input gluon with
$$\begin{aligned} f_0(x,k_t)=\alpha _s(k_t)\delta (x-x_0), \end{aligned}$$
(4)
where we take \(x_0=0.2\). Since the probability to have a large \(k_t\) gluon should be suppressed by the small QCD coupling, we have included in (4) the factor \(\alpha _s(k_t)\). We use the one-loop running coupling \(\alpha _s(k_t^2)\) with \(\Lambda _\mathrm{QCD}=0.15\) GeV, and the number of light quarks to be \(n_f=4\). Besides this, we account for the simple kinematical constraint—when the parton carries fraction \(x\) of the initial proton momenta, the transverse momentum \(k_t\) cannot exceed the value \(k_{t,\mathrm max}=\sqrt{xs}\), where \(\sqrt{s}\) is the initial energy.

It is natural to approximate the input by taking \(x_0=0.2\). The reasons are as follows. For BFKL evolution we have to consider small \(x\), but we would like to cover the largest possible rapidity interval. Therefore we start with \(x_0=0.2\), reserving a larger \(x\) interval for the valence quarks, and possible Good–Walker diffractive eigenstates [18], which describe low-mass diffractive dissociation. Moreover the typical DGLAP input gluon has a \((1-x)^5\) type distribution corresponding to a mean of \(x\) of about 0.2.

To include the effects of absorption (that is, the rescattering of intermediate partons along the ladder) we follow [19] and multiply the BFKL kernel \(\mathcal{K}\) of Eq. (3) by a canonical absorptive factor of the form \(\exp (-\lambda \Omega (y,k_t)/2)\) which depends on the rapidity, \(y=\ln (1/x)\) and the \(k_t\) of the current parton. Here \(\Omega \) is the optical density of the target gluon, while the factor \(\lambda \) accounts for the value of the triple-pomeron vertex, such that \(\lambda \Omega \) is the opacity of an incoming proton–‘current’ parton interaction.3 However, we must account for the absorption by both the incoming beam \((a)\) and the target \((b)\) protons interacting with intermediate partons. That is, actually the absorptive factor reads
$$\begin{aligned} S=\exp (-\lambda [\Omega ^b(y,k_t)+\Omega ^a(y',k_t)]/2), \end{aligned}$$
(5)
where \(y\) (\(y'\)) is the rapidity difference between the beam (target) proton and the current, intermediate gluon in the BFKL evolution. Denoting the rapidity separation between the beam and the target protons by \(Y\), we have \(y'=Y-y\).
The simplest absorptive effect comes from the triple-pomeron diagram shown in Fig. 1b. As in [19], we use the Leading Log expression for the BFKL triple-pomeron vertex, that is [8, 20, 21],
$$\begin{aligned} \lambda =N_c\alpha _S(k_t)\Theta (k'_t-k_t). \end{aligned}$$
(6)
The \(\Theta \)-function reflects the fact that (after averaging over the azimuthal angle) the large-size pomeron (i.e. the ladder with small \(k'_t\)) does not ‘see’ the small-size colourless object described by the BFKL pomeron component with \(k_t>k'_t\).
Note that the suppression factor, written in the form (5), includes not just the triple-pomeron diagram, but also a series of the multi-pomeron contributions generated by the vertices, \(g^n_m\), coupling \(n\) to \(m\) pomerons. Here we prefer to take the simple eikonal-like expression
$$\begin{aligned} g^n_m=\Omega (\lambda \Omega )^{n+m-2}, \end{aligned}$$
(7)
which satisfies the AGK cutting rules [22, 23]. However, this means that we have to replace the exponents \(\exp (-\lambda \Omega /2)\) in (5) by the factor
$$\begin{aligned} \frac{1-\exp (-\lambda \Omega )}{\lambda \Omega }. \end{aligned}$$
(8)
So now the absorptive factor (5) becomes
$$\begin{aligned}&S(y,y',k_t,k'_t)\nonumber \\&\quad =\frac{[1-\exp (-\lambda \Omega ^b(y,k_t))]}{\lambda \Omega ^b(y,k_t)} \frac{[1-\exp (-\lambda \Omega ^a(y',k_t))]}{\lambda \Omega ^a(y',k_t)}\nonumber \\ \end{aligned}$$
(9)
with the \(\lambda (k'_t,k_t)\) given by (6).
In terms of gluon density \(f(x,k_t)\), the ‘differential’ opacity \(\Omega ^b(y,k_t)\) of hadron \(b\) (corresponding to the contribution from the \(d\ln (k^2_t)\) interval) reads4
$$\begin{aligned} \lambda \Omega ^b(y,k'_t)=N_c\pi ^2\alpha _s(k'_t) \frac{f^b(y,k'_t)}{16\pi k^{'2}_t\ B_g}\ , \end{aligned}$$
(10)
where \(B_g/2\) is the \(t\)-slope of the initial “constituent gluon” form factor; we take5 \(B_g=1\) GeV\(^{-2}\). To obtain the full opacity we take the integral
$$\begin{aligned} \Omega (y) = \int _{k^2_t}\Omega (y,k'_t)\frac{dk^{'2}_t}{k^{'2}_t}, \end{aligned}$$
(11)
where the lower limit reflects the \(\Theta (k'_t-k_t)\) function in (6).
Since the opacity \(\Omega ^a(y,k_t)\) is proportional to \(f^a(y,k_t)\) we may write the evolution equation in rapidity \(y\), just in terms of opacities. Thus, finally, we obtain a system of two evolution equations. One equation evolving for \(\Omega ^b\) up from the target \((b)\) at \(y=0\), and one for \(\Omega ^a\) evolving down from the beam \((a)\) at \(y'=Y_k=\ln (s/k^{'2}_t)\). That is,
$$\begin{aligned} \frac{\partial \Omega ^b(y,k_t)}{\partial y}&= \frac{\alpha _s(k_t)}{2\pi }\int dk^{'2}_t S(y,y',k_t,k'_t)\nonumber \\&\times \,\mathcal{K}(k_t,k'_t)\Omega ^b(y,k'_t)\nonumber \\ \frac{\partial \Omega ^a(y',k_t)}{\partial y'}&= \frac{\alpha _s(k_t)}{2\pi }\int dk^{'2}_t S(y,y',k_t,k'_t)\nonumber \\&\times \,\mathcal{K}(k_t,k'_t)\Omega ^a(y',k'_t) \end{aligned}$$
(12)
for the evolution of gluon distributions from both the target and the beam initial hadrons (protons) in the absorptive (background) field of both hadrons. This system can be solved by iteration. In fact, it converges after just a few iterations.

3 The parton \(k_t\) distribution

The transverse momentum distribution at rapidity \(y\) has the form
$$\begin{aligned} \frac{{\text {d}}\sigma }{{\text {d}}k^2_t}\propto \frac{f^b(y,k_t)f^a(y'=Y-y,k_t)}{k^4_t}. \end{aligned}$$
(13)
The system of Eq. (12) was solved numerically by iteration, introducing an infrared cutoff \(k_0=0.5\) GeV; that is, assuming \(f(y,k_t<k_0)=0\). The resulting transverse momentum distributions are presented in Fig. 2. The solid lines are the predictions for the gluon distribution in the central plateau region (with rapidity \(y=Y/2\)), while the dashed lines correspond to distributions shifted to the fragmentation region of the incoming proton (i.e. initial gluon) with \(y=Y/6\). The \(y=Y/6\) curves are steeper and the corresponding mean transverse momentum is smaller than that in the centre (\(y=Y/2\)). As expected the distributions become flatter when the energy increases. However, at the Tevatron (thick black curves) and even at the 8 TeV LHC (thin black curve) we are still far from true saturation. Only at \(\sqrt{s}=100\) TeV do we predict an horizontal interval for \(k_t<2\) GeV. For comparison we present (by a dot-dashed blue line) the distribution expected at \(\sqrt{s}=100\) TeV if one neglects the absorptive effects, that is, we have the case when the survival factor \(S\equiv 1\) in (12). The distribution then decreases approximately linearly with increasing \(k_t\).
Fig. 2

The intermediate gluon distribution \(dN/dk^2_t\) in the centre of plateau, \(y=Y/2\), (solid lines) and near the edge of plateau at \(y=Y/6\) (dashed lines, shown for 2 and 100 TeV). The dot-dashed (blue) line shows the distribution at \(\sqrt{s}=100\) GeV generated if we neglect the absorptive effects

Next in Fig. 3 the rapidity dependence of mean transverse momenta, \(\langle k_t \rangle \) is shown for the Tevatron (\(\sqrt{s}=2\) TeV) and the LHC (\(\sqrt{s}=8\) TeV), and for \(\sqrt{s}=100\) TeV. The value of mean \(\langle k_t\rangle \) increases with energy, and it decreases as the rapidity approaches the position of the initial hadron.
Fig. 3

The mean transverse momentum, \(\langle k_t \rangle \), of the gluon versus the pseudorapidity, \(\eta \), of the intermediate gluons

4 How to measure the \(k_t\) distribution

Note that the predicted values of \(\langle k_t\rangle \) are of the same ‘order of magnitude’, but smaller than, the value of the \(k_\mathrm{min}\) cutoff used in the PYTHIA Monte Carlo, which is based on DGLAP evolution. However, we have to recall that (a) these are not exactly the same quantities and (b) here we have used a simplified model based on the LO BFKL kernel.6 The advantage of this model is that it is sufficiently transparent and practically has no free parameters. The only exceptions are the starting values of \(x_0=0.2\) and \(k_0=0.5\) GeV and the slope \(B_g=1\) GeV\(^{-2}\) of the initial ‘constituent’ gluon. The parameters are not chosen to describe the data, but simply taken to have physically reasonable values. Besides this, there may be some ‘intrinsic’ transverse momentum of the initial gluon which will enlarge the final value of \(\langle k_t\rangle \).

We should emphasise that the partonic \(k_t\) distribution, although not directly observable, drives all soft high-energy interactions. Clearly it would be interesting to measure the gluon’s \(\langle k_{g,t}\rangle \) experimentally. Can this be done? The problem is that actually we never observe partons, but only the final secondary hadrons, which are mainly pions. Unfortunately the distributions of light hadrons (such as pions, kaons) are strongly affected by final-state interactions: that is, by hadronisation, confinement and the decay of resonances. In particular, the \(p_t\) distribution of secondary pions strongly depends on the possible colour re-connection. Therefore it appears better to study the distributions of mesons which contain one heavy quark. Due to the strong leading particle effect [11, 12, 13], the \(p_t\) distribution of these mesons is close to that of the heavy quark. Since heavy quarks are mainly produced by the \(gg\rightarrow Q\bar{Q}\) subprocess, we may expect that (modulo some smearing due to hadronisation when the heavy quark picks up a light antiquark) the mean momentum of such a meson should carry the momentum of the parent gluon. Final-state interactions and resonance decays do not appreciably distort the \(p_t\) distributions of these heavy mesons.

On one hand, it might be the best to measure the \(p_t\) distributions of heavy B-mesons, where the leading particle effect is more pronounced. On the other hand, the \(b\)-quark already receives a rather large
$$\begin{aligned} k_t=k_\mathrm{background}\sim m_b \end{aligned}$$
(14)
from the hard \(gg\rightarrow b\bar{b}\) subprocess and it may be hard to observe the variation of the incoming gluon \(\langle k_{g,t}\rangle \) on the top of this large ‘background’, \(k_\mathrm{background}\). Therefore, it seems better to detect D-mesons where the value of \(k_\mathrm{background}\sim m_c\) is comparable with the expected gluon’s \(\langle k_{g,t}\rangle \). We would hope to observe the growth of \(\langle p_{D,t}\rangle \) with energy at fixed rapidity, and a decrease of \(\langle p_{D,t}\rangle \) with pseudorapidity7 at a fixed energy. The last effect can be observed by a comparison of the CMS/ATLAS data at \(\eta =0\) with the LHCb data at \(\eta =3\)–4.

Moreover, note that it possible to do better. We could suppress the \(k_\mathrm{background}\) contribution generated into the ’hard’ \(gg\rightarrow Q\bar{Q}\) subprocess if the transverse momenta of both heavy mesons (\(D\) and \(\bar{D}\) or \(B\) and \(\bar{B}\)) are measured. In such a case the transverse momentum of the \(Q\bar{Q}\) pair is simply equal to the momentum of the parent gluon pair. Of course, we cannot avoid the smearing due to hadronisation, but it is not so large since it is controlled by the confinement scale and not by the heavy quark mass. So it would be good to measure the vector sum of the momenta of the two heavy mesons, or just the coplanarity between the two heavy mesons. Non-complanarity should increase with energy, but decrease with \(\eta \).

Another attractive measurement is to compare the \(p_t\) of the secondaries produced in the diffractive dissociation with those from non-diffractive inelastic events. It is usually expected (see, for example, [26, 27]), that the spectra of particles produced in proton diffractive dissociation into a high-mass \((M_X)\) state, are similar to that in normal inelastic events taken at an energy \(\sqrt{s}=M_X\). That is in the situation when the energies of the final states are the same. On the contrary, in the picture described above, even in the case of dissociation, the \(p_t\) distribution of secondaries should be driven by the parton’s \(k_t\) formed by the whole initial energy \(\sqrt{s} \gg M_X\). That is, it does not matter whether the events have a large rapidity gap (LRG) or not. One consequence (see, also, [28]) is that in proton diffractive dissociation to a large \(M_X\) system (but still \(M_X\ll \sqrt{s}\)) the dissociation events, especially near the edge of the LRG, are expected to have a larger \(p_t\) than those in a normal inelastic \(pp\)-collision at \(\sqrt{s}=M_X\); modulo to possible hadronisation effects. Moreover, the rapidity dependence of the \(p_t\) spectra in LRG events are also similar to that in the inelastic interaction at full proton–proton energy \(\sqrt{s}\), and not to the inelastic events with the proton–proton energy equal to \(M_X\). Again, to reduce the effects of hadronisation, it would be better to make the comparison by measuring the distributions of \(D\)-mesons both in inelastic and high-mass dissociation events.

5 Conclusions

The transverse momentum distribution of partons plays a pivotal underlying role both in the spectral shape of secondaries and in the asymptotic behaviour of high-energy proton–proton collisions. At first sight, just from dimensional arguments, we expect \(d\sigma /dk_t^2 \propto 1/k^4_t\). That is, the major contribution should come from low \(k_t\), close to the cutoff (\(\lesssim \)0.3 GeV) provided by confinement. On the contrary, to describe the data, it was necessary to introduce a much higher cutoff, \(k_\mathrm{min}\), in the hard matrix element of the order of a few GeV, with a value that increases with collider energy, like \(s^{0.12}\). Actually such a \(k_\mathrm{min}\) was obtained by tuning the Monte Carlo generators [5, 6], but clearly it should be of theoretical origin. Moreover, \(k_\mathrm{min}\) of the order of a few GeV should be explained in terms of perturbative QCD.

Here, we use a model based on the LO BFKL equation, supplemented by absorptive multi-pomeron corrections. The original BFKL equation includes diffusion in log\(k_t\), with, at each step of the evolution, the possibility that \(k_t\) may increase or decrease with equal probabilities. However, strong absorption of low \(k_t\) partons leads to a growth of \(\langle k_t \rangle \) with collider energy. We demonstrate that this effect naturally explains the observed energy behaviour of the effective cutoff, \(k_\mathrm{min}\).

We did not perform a fit to the data, but show, at a qualitative level, that a simplified model based on leading order perturbative QCD with a few physically motivated parameters, produces a reasonable \(k_t\) distribution of the partons. We present the expected \(k_t\) distributions at different collider energies and the dependence of \(\langle k_t\rangle \) on the energy and rapidity of the parton.

Although the \(k_t\) of the parton is not directly observable, we discuss the possibility to experimentally verify these predictions. One way, is to measure the \(p_t\) distributions of mesons containing a heavy \(c\) or \(b\) quark, or better to measure \(D\bar{D}\) or \(B\bar{B}\) meson pairs. Another possibility is to compare the \(p_t\) spectra of diffractive dissociation events with those of non-diffractive inelastic scattering.

Footnotes

  1. 1.

    This cutoff is very similar to the so-called ‘saturation’ momentum scale widely discussed for PDFs at low \(x\). It was first mentioned in [7, 8], and then considered in many papers based on the Balitsky–Kovchegov (BK) equation, see, for example, the reviews in [9, 10]. In comparison with the calculations based on the BK equation, here we account for the interaction of the (current) intermediate parton with both the beam and the target protons [see Eqs. (5) and (9) below].

  2. 2.

    Here we have already integrated over the azimuthal angle \(\phi \) assuming, similar to the DGLAP case, a flat \(\phi \) dependence of \(f\); that is, we consider the zero harmonic, which corresponds to the trajectory with the rightmost intercept.

  3. 3.

    Recall that, in the eikonal framework, exp\((-\Omega )\) is the probability of no inelastic interaction. Since we consider the amplitude, and not the cross section, we put \(\Omega /2\) in (5), rather than the full opacity \(\Omega \).

  4. 4.

    This equation follows after integrating Eq. (17) of [19] over the impact parameter, \(b\), or from [20].

  5. 5.

    There are several arguments in favour of the effective slope \(B_g\) being of the order of 1 GeV\(^{-2}\); that is, in favour of the small-size ‘hot-spot’ transverse area occupied by our gluon amplitude. The first reason, is the small radius of the gluonic form factor of the proton calculated using QCD sum rules [24]. The next argument is the small value of the effective slope of the pomeron trajectory observed experimentally. Further evidence is the success of the additive quark model, \(\sigma (\pi p)/\sigma (pp) \simeq 2/3\). Finally, in the explicit calculation of our amplitude, following [25], we indeed found an almost constant slope \(B_g \simeq 0.9 ~\mathrm GeV^{-2}\) for the present collider energy interval.

  6. 6.

    Surprisingly, with the same parameters, LO BFKL (supplemented by the simple kinematic constraint and absorptive multi-pomeron effects) leads to an effective gluon–gluon (hot-spot) interaction that increases like \(s^{0.15}\) in the present collider energy interval, which is in reasonable agreement with the intercept needed to describe the experimental data.

  7. 7.

    Measured in the laboratory frame (\(\eta =-\ln \tan (\theta _\mathrm{lab}/2)\)).

Notes

Acknowledgments

MGR thanks the IPPP at the University of Durham for hospitality. This work was supported by the RSCF Grant 14-22-00281.

References

  1. 1.
    L.N. Lipatov, Sov. Phys. JETP 63, 904 (1986)Google Scholar
  2. 2.
    L.N. Lipatov, Zh. Eksp, Teor. Fiz. 90, 1536 (1986)Google Scholar
  3. 3.
    V. Khachatryan et al., CMS Collaboration, Phys. Rev. Lett. 105, 022002 (2010)Google Scholar
  4. 4.
    G. Aad et al., ATLAS Collaboration, New J. Phys. 13, 053033 (2011)Google Scholar
  5. 5.
    T. Sjostrand, S. Mrenna, P.Z. Skands, Comput. Phys. Commun. 178, 852 (2008)ADSCrossRefGoogle Scholar
  6. 6.
    A. Buckley, J. Butterworth, S. Gieseke, D. Grellscheid, S. Hoche, H. Hoeth, F. Krauss, L. Lonnblad et al., Phys. Rep. 504, 145 (2011)ADSCrossRefGoogle Scholar
  7. 7.
    L.V. Gribov, E.M. Levin, M.G. Ryskin, Nucl. Phys. B 188, 555 (1981)ADSCrossRefGoogle Scholar
  8. 8.
    L.V. Gribov, E.M. Levin, M.G. Ryskin, Phys. Rep. 100, 1 (1983)ADSCrossRefGoogle Scholar
  9. 9.
    A.H. Mueller, D.N. Triantafyllopoulos, Nucl. Phys. B 640, 331 (2002)ADSCrossRefMATHGoogle Scholar
  10. 10.
    Y.V. Kovchegov, E. Levin, Quantum Chromodynamics at High Energy, Cambridge Monographs on Particle Physics, Nuclear Physics and Vosmology, vol. 33 (Cambridge University Press, Cambridge, 2012)Google Scholar
  11. 11.
    Y.L. Dokshitzer, V.A. Khoze, S.I. Troian, J. Phys. G 17, 1481 (1991)ADSCrossRefGoogle Scholar
  12. 12.
    Y.L. Dokshitzer, V.A. Khoze, S.I. Troian, Phys. Rev. D 53, 89 (1996)Google Scholar
  13. 13.
    M. Cacciari, E. Gardi, Nucl. Phys. B 664, 299 (2003)ADSCrossRefGoogle Scholar
  14. 14.
    V.S. Fadin, E.A. Kuraev, L.N. Lipatov, Phys. Lett. B60, 50 (1975)ADSCrossRefGoogle Scholar
  15. 15.
    E.A. Kuraev, L.N. Lipatov, V.S. Fadin, Sov. Phys. JETP 44, 443 (1976)ADSGoogle Scholar
  16. 16.
    E.A. Kuraev, L.N. Lipatov, V.S. Fadin, Sov. Phys. JETP 45, 199 (1977)ADSMathSciNetGoogle Scholar
  17. 17.
    I.I. Balitsky, L.N. Lipatov, Sov. J. Nucl. Phys. 28, 822 (1978)Google Scholar
  18. 18.
    M.L. Good, W.D. Walker, Phys. Rev. 120, 1857 (1960)ADSCrossRefGoogle Scholar
  19. 19.
    M.G. Ryskin, A.D. Martin, V.A. Khoze, Eur. Phys. J. C 71, 1617 (2011)ADSCrossRefGoogle Scholar
  20. 20.
    J. Bartels, M. Wusthoff, Z. Phys. C 66, 157 (1995)ADSCrossRefGoogle Scholar
  21. 21.
    I. Balitsky, Nucl. Phys. B 463, 99 (1996)ADSCrossRefGoogle Scholar
  22. 22.
    V.A. Abramovsky, V.N. Gribov, O.V. Kancheli, Yad. Fiz. 18, 595 (1973)Google Scholar
  23. 23.
    V.A. Abramovsky, V.N. Gribov, O.V. Kancheli, Sov. J. Nucl. Phys. 18, 308 (1974)Google Scholar
  24. 24.
    V.M. Braun, P. Gornicki, L. Mankiewicz, A. Schafer, Phys. Lett. B302, 291 (1993)Google Scholar
  25. 25.
    E.M. Levin, M.G. Ryskin, Z. Phys. C48, 231 (1990)Google Scholar
  26. 26.
    J. Whitmore, Phys. Rep. 27, 187 (1976)ADSCrossRefGoogle Scholar
  27. 27.
    A.B. Kaidalov, Phys. Rep. 50, 157 (1979)ADSCrossRefGoogle Scholar
  28. 28.
    M.G. Ryskin, A.D. Martin, V.A. Khoze, J. Phys. G 38, 085006 (2011)ADSCrossRefGoogle Scholar

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Authors and Affiliations

  1. 1.Institute for Particle Physics PhenomenologyUniversity of DurhamDurhamUK
  2. 2.Petersburg Nuclear Physics InstituteNRC Kurchatov InstituteGatchinaRussia

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