Advances in High Energy Physics

Volume 2019, Article ID 1901659, 6 pages

https://doi.org/10.1155/2019/1901659

## Quark-Antiquark Potential from a Deformed AdS/QCD

^{1}Departamento de Física Teórica, Universidade do Estado do Rio de Janeiro, 20.550-900 - Rio de Janeiro-RJ, Brazil^{2}Departamento de Física and Mestrado Profissional em Práticas da Educação Básica (MPPEB), Colégio Pedro II, 20.921-903 - Rio de Janeiro-RJ, Brazil^{3}Instituto de Física, Universidade Federal do Rio de Janeiro, 21.941-972 - Rio de Janeiro-RJ, Brazil

Correspondence should be addressed to Henrique Boschi-Filho; moc.liamg@ihcsobh

Received 26 July 2018; Revised 22 December 2018; Accepted 30 December 2018; Published 13 January 2019

Academic Editor: George Siopsis

Copyright © 2019 Rodrigo C. L. Bruni et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP^{3}.

#### Abstract

In this work we calculate the static limit of the energy for a quark-antiquark pair from the Nambu-Goto action using a holographic approach with a deformed AdS space, with warp factor . From this energy we derive the Cornell potential for the quark-antiquark interaction. We also find a range of values for our parameters which fits exactly the Cornell potential parameters. In particular, setting the zero energy of the Cornell potential at 0.33 fermi, we find that GeV and .

#### 1. Introduction

The quark-antiquark potential has been a very useful tool for the investigation of strong interactions and quark confinement. This potential can be used, for example, to analyze the transition between the confined and deconfined phases of matter (see, for instance, [1]).

Recently, efforts have been made to obtain the quark-antiquark potential [2–11] using the well-known AdS-CFT correspondence. For another approach using effective string theory, see, for instance, [12]. This correspondence was originally formulated as a mapping of correlation functions of a superconformal Yang-Mills theory defined on the boundary of the AdS space and a string theory living in its bulk. It works in such a way that a strongly coupled regime on the boundary theory is mapped into a weakly coupled one in the bulk [13–17].

However, since the original formulation of the correspondence is based on a conformal field theory, which has no characteristic scale, the confining behavior of the potential is not contemplated once confinement implies a typical length scale.

In order to describe both the confining and nonconfining behaviors, it becomes necessary to break the conformal invariance of the theory. There are various ways of doing so but we mention just two of them: the hardwall [18–24] and the softwall [25–28] models which break conformal invariance introducing a cutoff in the action. Inspired by [6], here we break the conformal invariance modifying the background metric instead of the bulk action. So the metric is given bywhere is the AdS radius, , where is the holographic coordinate while with represents an Euclidean space in four dimensions. The warp factor that we consider here in this work is given byin which has dimensions of inverse length and is a dimensionless number. We will keep these constants arbitrary until Section 3, where we relate our results to phenomenology of the quark-antiquark potential. Note that, if we restrict , we reobtain the results of [6].

The main goal of this work is to calculate the energy configuration for a quark-antiquark pair from the Nambu-Goto action using a holographic approach within the deformed metric (1) with the warp factor given by (2). From this energy we will obtain the Cornell potential [29–33] (for excellent reviews of the Cornell potential see [34, 35]):and also find a range of values for the parameters and which describe in order to fit this potential.

This work is organised as follows. In Section 2, using the warp factor , we compute the separation and the energy of the quark-antiquark pair using the Wilson loop from the AdS/CFT correspondence. In Section 3, we discuss the matching of our parameters and to fit the Cornell potential. Finally, in Section 4, we present our comments and conclusions. We also include an appendix where we give some details of the calculation of the energy and the separation distance of the string.

#### 2. The Wilson Loop and the Quark Potential

The starting point of our calculations involves the Wilson loop. For convenience we choose one circuit corresponding to a rectangular spacetime loop with temporal extension and spatial extension in the association with the area of the string worldsheet that lives in the AdS space, whose boundary is just the flat spacetime in 4 dimensions where the loop is defined [2, 3].

So, following this prescription, we just have to calculate the Nambu-Goto action of a string with the endpoints (identified as the quark and antiquark) fixed at , assuming a “U-shape” equilibrium configuration in the bulk of deformed AdS.

Assuming also that the string configuration is, by hypothesis, static, i.e., it moves in the interior of the deformed AdS without change in its shape, one can show that the interquark separation and energy for the type of metric (1) are, respectively, given by (see the appendix for details)Note that is the minimum of the coordinate and corresponds to the bottom of the U-shape curve.

The form of (4) and (5) is very convenient because it makes explicit that the expressions of energy and separation distance depend only on the warp factor chosen for the metric and the value of .

It is useful to rewrite the integrals (4) and (5) in terms of a dimensionless variable. If we define , the integrals becomewhich makes explicit the dimensions of and since the integrals are now dimensionless, and where we identify . Note also that the ratio is dimensionless.

Now we introduce the dimensionless parameter such that (6) and (7) becomewhere has the dimension of energy. Let us analyze the above expressions when and , which are the interesting physical limits since for one has , while for one has , as we are going to discuss below.

##### 2.1. Calculation of

###### 2.1.1. Close to Zero

If we express the integrand in (8) as a power series in centered at zero, to first order in , and integrate it, we obtainwhere the above result is valid only if ; otherwise the integral does not converge.

Substituting this result in (8) and grouping terms proportional to , one findsHere we have defined the dimensionless number and function .

###### 2.1.2. Close to 2

If we repeat the procedure of last subsection for now centered at 2, we will not be able to achieve an analytic expression for the integral. We note however that the integral of (8) is dominated by . We thus expand the integrand around to first order and integrate it, obtaining the following.

As the first logarithm of (12) diverges when , one would expand again around up to first order. However, since terms of order in the expansion will not contribute to the functional form of the Cornell potential and we are extracting just the leading behavior of (8) for , we can safely neglect contributions of order in the aforementioned expansions, obtainingwhich, due to (8), leads toAs mentioned above, the limit implies .

##### 2.2. Calculation of the Energy

Before we calculate the integral in (9), let us point out that it diverges as when . This becomes clear if one analyzes the series expansion of the integrand in close to 0 and 2.

So, we choose the renormalization of (9) assuch that this energy expression is finite and now we can analyze again the limits of close to 0 and 2.

###### 2.2.1. Close to Zero

Expanding the integrand in (15) with respect to , centered at zero, we find

so that the renormalized energy iswhere we defined the dimensionless function .

Writing the prefactor as a function of (c.f. (11)), substituting in (17), and keeping only linear terms in , we getwhere we defined the dimensionless number . Using (11) we can rewrite in terms of and :

Substituting this result in (18) and keeping in mind that is equivalent to the regime of short distances, one can safely disregard terms proportional to in comparison with the terms proportional to . Then, we obtainwhere we defined the function , with dimensions of .

###### 2.2.2. Close to 2

In this section we are going to calculate the renormalized energy for close to 2. Repeating the procedure employed in Section 2.1.2, i.e., rewriting all the integrand in (15) inside the square rootand expanding this integrand with respect to centered at 1, to second order we findFor the above expression to be real, the first two terms must be positive and the last one must be negative which implies, respectively, that and . Now, integrating (22), one has

Keeping only terms in lowest order of and substituting in the denominator of above expression, we get from (15)where we have used the relation between and given by (14) and defined .

#### 3. Phenomenology

Summarizing the results of the last section, the renormalized energies (20) and (24) in terms of the separation are given bywithThe precise definition of , given after (20), will not be needed here since in this section we are going to disregard the term proportional to in comparison with the term of order , once and in (25) .

Now we are going to fit the constants of our model with the phenomenological constants of the Cornell potential (3) with and [29–33] (for excellent reviews of the Cornell potential see [34, 35]).

First of all, we fix the dimensionless ratio from the slope of the linear potential at long distances, where the stringy picture is more reliable. Since this regime is equivalent to , we compare (3) with (26), which leads to the condition and therefore

Next, we compare the expression (25) with (3), finding , so that eliminating the ratio , one obtains

The above equation can be solved graphically for given values of : we present some of these solutions in Figure 1, for the interval .