<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2013.412195</article-id><article-id pub-id-type="publisher-id">JMP-40913</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Critical Line Back-Bending Induced either by Finite &lt;i&gt;N&lt;sub&gt;c&lt;/sub&gt;&lt;/i&gt; Corrections or by a Repulsive Vector Channel
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>obson</surname><given-names>Z. Denke</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Juan</surname><given-names>Camilo Macias</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marcus</surname><given-names>Benghi Pinto</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>1Departamento de Física, Universidade Federal de Santa Catarina, Florianópolis, Brazil
2Departamento de Física, Funda??o Universidade Regional de Blumenau, Blumenau, Brazil </addr-line></aff><aff id="aff2"><addr-line>Departamento de Física, Universidade Federal de Santa Catarina, Florianópolis, Brazil</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>r.denke@posgrad.ufsc.br(OZD)</email>;<email>marcus@fsc.ufsc.br(MBP)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>06</day><month>12</month><year>2013</year></pub-date><volume>04</volume><issue>12</issue><fpage>1583</fpage><lpage>1590</lpage><history><date date-type="received"><day>August</day>	<month>28,</month>	<year>2013</year></date><date date-type="rev-recd"><day>September</day>	<month>29,</month>	<year>2013</year>	</date><date date-type="accepted"><day>October</day>	<month>26,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p><html>
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   We analyze the two flavor version of the Nambu-Jona-Lasinio model with a repulsive vector coupling (G<sub>V</sub>), at finite temperature and quark chemical potential, in the strong scalar coupling (G<sub>s</sub>) regime. Considering G<sub>V</sub> = 0, we review how finite N<sub>c</sub> effects are introduced by means of the Optimized Perturbation Theory (OPT) which adds a <img alt="" src="Edit_fd74dcfc-c735-4b24-a53a-26ac778df5b1.bmp" width="70" height="18" /> term to the thermodynamical potential. This 1/ N<sub>c</sub> suppressed term is similar to the <img alt="" src="Edit_d4fbd2e8-ef23-4ac0-974c-b05d94ce2f18.bmp" width="44" height="18" /> contribution obtained at the large-N<sub>c</sub> limit when G<sub>V</sub> ≠ 0. Then, scanning over the quark current mass values, we compare these two different model approximations showing that both predict the appearance of two critical points when chiral symmetry is weakly broken. By mapping the first order transition region in the chemical potential-current mass plane, we show that, for low chemical potential values, the first order region shrinks as μ increases but the behavior gets reversed at higher values leading to the back-bending of the critical line. This result, which could help to conciliate some lattice results with model predictions, shows the important role played by finite N<sub>c</sub> corrections which are neglected in the majority of the works devoted to the determination of the QCD phase diagram. Recently the OPT, with G<sub>V</sub> = 0, and the large-N<sub>c</sub> approximation, with G<sub>V</sub> ≠ 0, were compared at zero temperature and finite density for one quark flavor only. The present work extends this comparison to finite temperatures, and two quark flavors, supporting the result that the OPT finite N<sub></sub> 
 
</html></p></abstract><kwd-group><kwd>QCD Phase Diagram; NJL Model</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Although most of the results obtained up to now seem to support the quantum chromodynamics (QCD) critical point (CP), an interesting observation against its existence comes from the numerical simulations of QCD at imaginary chemical potential by de Forcrand and Philipsen [1-3] which shows that the region of quark masses (m<sub>c</sub>) where the transition is presumably of the first order (for quark masses smaller than the physical ones), tends to shrink for small positive values of the chemical potential as shown in the upper panel of <xref ref-type="fig" rid="fig1">Figure 1</xref>. Conversely, according to models supporting the critical point, the first order region should expand when the chemical potential increases, so that the physical quark mass point hits the critical line at some finite value of the temperature and chemical potential as shown in the bottom panel of <xref ref-type="fig" rid="fig1">Figure 1</xref>. A possible explanation for the disagreement between the “exotic” scenario (<xref ref-type="fig" rid="fig1">Figure 1</xref>, upper panel) and the “standard” scenario (<xref ref-type="fig" rid="fig1">Figure 1</xref>, bottom panel) has been given in [4,5] where it was suggested that a strong (repulsive) vector coupling may account for the initial shrinkage of the first order region, that would then start expanding again at larger values of the chemical potential leading to the back-bending of the critical surface and the recovery to the CP at the physical quark mass values. As a result, two critical points should appear for a given range of (small) quark masses, as argued by Bowman and Kapusta [<xref ref-type="bibr" rid="scirp.40913-ref6">6</xref>] who investigated the Linear Sigma Model (LSM) including thermal fluctuations and considered small values for the pion mass. A pictorial view of this peculiar situation is given by <xref ref-type="fig" rid="fig2">Figure 2</xref> which illustrates a possible back-bending scenario in the two-flavor case. In the more traditional T − μ plane, these two critical points are located at the end of two first order transi-</p><p>tion lines where one of them represents the usual line which starts at zero temperature and chemical potential of the order of the constituent quark mass while the other is an unusual line which starts at zero chemical potential and high temperature [6,7].</p><p>In [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] the author has considered the three flavor Nambu-Jona-Lasinio model (NJL) at large-N<sub>c</sub> with an explicit repulsive vector interaction, with coupling G<sub>V</sub>, in order to produce a back-bending that would conciliate the lattice results obtained by de Forcrand and Philipsen with most model predictions. It is well known that within the NJL this type of interaction weakens the first order transition line [<xref ref-type="bibr" rid="scirp.40913-ref8">8</xref>] in opposition to the scalar coupling <img src="5-7501513\66c039d4-2221-4a01-854d-0ffeeabb5e0f.jpg" /> which tends to favor the appearance of first order phase transitions [<xref ref-type="bibr" rid="scirp.40913-ref9">9</xref>] . The explicit presence of a vector term was decisive in order to produce the back-bending scenario within the large-N<sub>c</sub> application of [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] . It was explained that the net effect produced by a repulsive vector channel is to add a term like −G<sub>V </sub>r<sub>q</sub><sup>2</sup> (here ρ<sub>q</sub> represents the quark number density) to the pressure and as a result the size of the first order covers a smaller range of temperatures as compared to the G<sub>V</sub> = 0 case.</p><p>At the same time, the value of the coexistence chemical potential for a given temperature occurs at a higher value when G<sub>V</sub> ≠ 0 and, as a consequence, the critical end point happens at smaller temperatures to be higher chemical potentials than in the case of vanishing G<sub>V</sub>. Although such a vector term is known to be important at high densities in theories such as the Walecka model for nuclear matter, its consideration is more delicate within a non renormalizable model such as the NJL where usually the integrals are regulated by a momentum cut-off, Λ. Within this model, G<sub>S</sub> and Λ are usually fixed to reproduce the pion mass<img src="5-7501513\d4946bf5-bd4a-4bb0-8260-8e14b98b866c.jpg" />, the pion decay constant</p><p><img src="5-7501513\4b7ea41c-b6aa-4d0f-9181-05740be2ed41.jpg" />and the quark condensate</p><p><img src="5-7501513\f7c39f6f-48fd-4bc7-94e6-4feb82bc5687.jpg" />which yields Λ ~ 560 - 670 MeV, G<sub>S </sub>Λ<sup>2</sup> ~ 2 - 3.2 and m<sub>c</sub> ~ 5 - 5.6 MeV (see [<xref ref-type="bibr" rid="scirp.40913-ref10">10</xref>] for a complete discussion).</p><p>However, fixing G<sub>V</sub> poses and additional problem since this quantity should be fixed using the ρ meson mass which, in general, happens to be higher than the maximum energy scale set by Λ. Then, G<sub>V</sub> is usually considered to be a free parameter whose estimated value ranges between 0.25 G<sub>S</sub> and 0.5G<sub>S</sub> [11,12].</p><p>Alternatively, when going beyond the large-N<sub>c</sub> (or mean field) level one may induce quantum (loop) corrections which mimic the physical effects caused by a classical (tree) term such as G<sub>V</sub>. This is precisely what has been observed in an application of the nonperturbative Optimized Perturbation Theory (OPT) method to the two flavor NJL model with vanishing G<sub>V</sub> [<xref ref-type="bibr" rid="scirp.40913-ref13">13</xref>] . The OPT results for phase diagram for this model show that <img src="5-7501513\ee529711-b8f8-4205-afa5-c18375786f3c.jpg" /> corrections induced by this approximation reproduce the same qualitative features obtained by considering the model at large-N<sub>c</sub> with an explicit repulsive vector channel. The reason is that the OPT two loop contributions add a term like <img src="5-7501513\244fb8d9-c374-412a-9182-f84ff65a0f18.jpg" /> to the pressure.</p><p>The relationship between the OPT, at G<sub>V</sub> = 0, and the large-N<sub>c</sub> approximation, at G<sub>V</sub> ≠ 0, has been recently investigated in great detail in the framework of the abelian NJL at finite densities and zero temperature in [<xref ref-type="bibr" rid="scirp.40913-ref14">14</xref>] . In the context of the eventual back-bending behavior of the critical line in the μ − m<sub>c</sub> plane, the OPT has also been previously employed with success in [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] . There, the strategy was to use very high values for G<sub>S</sub> in order to obtain a T − μ phase diagram dominated by first order chiral transitions only.</p><p>Then, the OPT with its <img src="5-7501513\226ed3fa-49fa-46a9-bb27-730557d592d7.jpg" /> term was used at different quark mass values showing that, in this case, two critical points emerge at low m<sub>c</sub> due to the weakening of the first order line at intermediate μ values leading to the back-bending behavior observed in [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] without the need to explicitly include a vector channel in the lagrangian density.</p><p>Note that a repulsive vector type of coupling was not explicitly considered in the two flavor LSM application performed by Bowman and Kapusta which, on the other hand, was carried out beyond the mean field level through the consideration of thermal fluctuations.</p><p>In the present work, we extend the comparison between the OPT (at G<sub>V</sub> = 0) and the large-N<sub>c</sub> approximation (at G<sub>V</sub> ≠ 0) to the non abelian NJL model at finite temperature and density in the strong coupling and small quark mass regime showing that, as expected, both methods agree from the qualitative point of view leading to a back-bending which would be completely missed by a standard large-N<sub>c</sub> evaluation.</p><p>Our results also emphasize the importance played by <img src="5-7501513\876126af-7be4-4598-bc1d-96d64afbf7ef.jpg" /> terms which are easily taken into account by the OPT so that this method may be viewed as a robust alternative to investigate nonperturbative effects related to the chiral transition of strongly interacting matter. The work is organized as follows. In the next section, we perform a large-N<sub>c</sub> application to the two flavor NJL version in the strong coupling regime for the G<sub>V</sub> ≠ 0 case. In Section 3 we review the OPT results, at G<sub>V</sub> = 0, which were originally obtained in [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>]. We then compare, in Section 4, the analytical and numerical results obtained with the two different model approximations. Our conclusions are presented in Section 5.</p></sec><sec id="s2"><title>2. The NJL in the Strong Coupling Regime</title><p>The standard version of the two flavor Nambu-JonaLasinio model lagrangian density L with a repulsive vector channel reads [10,15]</p><disp-formula id="scirp.40913-formula114701"><label>(1)</label><graphic position="anchor" xlink:href="5-7501513\cc453418-d909-49ca-ab7a-ada937c6db0c.jpg"  xlink:type="simple"/></disp-formula><p>where y (a sum over flavors and color degrees of freedom is implicit) represents a flavor isodoublet (u and d type of quarks) N<sub>c</sub>-plet quark fields while <img src="5-7501513\55a81db6-3aa0-4301-beae-2a3e0ad7168b.jpg" /> are isospin Pauli matrices.</p><p>As emphasized in [<xref ref-type="bibr" rid="scirp.40913-ref16">16</xref>] , the introduction of a repulsive vector interaction term of the form <img src="5-7501513\d2efebe0-af22-4761-bda2-9a0db14eaecc.jpg" /> in Equation (1) is also allowed by the chiral symmetry. Such a term can become important at finite densities, generating a saturation mechanism depending on the vector coupling strength that provides better matter stability [10,16]. Here, we will show that this term also influences the phase diagram, especially at the low temperature and high density region. A standard parametrization for this model is Λ = 587.9 MeV, G<sub>S </sub>Λ<sup>2</sup> = 2.44, and m<sub>c</sub> = 5.6 MeV so that, with these inputs, one obtains f<sub>π</sub> = 93 MeV, m<sub>π</sub> = 135 MeV, and M = 400 MeV at T = 0, and μ = 0 [<xref ref-type="bibr" rid="scirp.40913-ref10">10</xref>] .</p><p>However, as will be shown in the next subsection, in order to simulate the back-bending behavior in the present model we will keep Λ = 587.9 MeV considering <img src="5-7501513\7b40d17e-292f-4831-8eaa-da5136596ec2.jpg" /> while varying the current quark mass from m<sub>c</sub> = 0 to m<sub>c</sub> = m<sub>phys</sub>= 5.6 MeV. As discussed in [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] this nonstandard choice does not affect very much the predicted values for observables such as f<sub>π </sub>, m<sub>π</sub> and<img src="5-7501513\2b2f98fb-daef-4dd9-89cc-58bafeb2b2a5.jpg" />. On the other hand the quark effective mass, which is directly proportional to G<sub>S</sub>, assumes very high values (around 800 MeV &gt; Λ). However, this is not a problem for our present purpose of simulating the back-bending in a qualitative way (see [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] for a more complete discussion).</p><sec id="s2_1"><title>2.1. Thermodynamical Potential at Large-N<sub>c</sub> with Finite G<sub>V</sub> Contributions</title><p>The large-N<sub>c</sub> (or MFA) evaluation of the thermodynamical potential within this model is standard and yields [<xref ref-type="bibr" rid="scirp.40913-ref10">10</xref>]</p><disp-formula id="scirp.40913-formula114702"><label>(2)</label><graphic position="anchor" xlink:href="5-7501513\3348e6f5-521f-4436-b3d3-18b31c3e2ed4.jpg"  xlink:type="simple"/></disp-formula><p>where the dressed “free gas” term is given by</p><disp-formula id="scirp.40913-formula114703"><label>(3)</label><graphic position="anchor" xlink:href="5-7501513\564cd5f7-0116-4222-b561-c2c861332d43.jpg"  xlink:type="simple"/></disp-formula><p>the scalar density is given by</p><disp-formula id="scirp.40913-formula114704"><label>(4)</label><graphic position="anchor" xlink:href="5-7501513\3876529d-84ef-4a58-b6bb-5d64745ad377.jpg"  xlink:type="simple"/></disp-formula><p>and the quark number density is given by</p><disp-formula id="scirp.40913-formula114705"><label>(5)</label><graphic position="anchor" xlink:href="5-7501513\4ea11c3c-d362-4be4-a5a8-694ab6b3e175.jpg"  xlink:type="simple"/></disp-formula><p>The integrals appearing in the above equations are defined by</p><disp-formula id="scirp.40913-formula114706"><label>(6)</label><graphic position="anchor" xlink:href="5-7501513\e9407a8c-8c71-4895-89ef-a0f02d5c02b8.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.40913-formula114707"><label>(7)</label><graphic position="anchor" xlink:href="5-7501513\17e38115-888b-4af5-8b79-0986212208a6.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.40913-formula114708"><label>(8)</label><graphic position="anchor" xlink:href="5-7501513\7ee9a90c-3553-46c5-a9ca-6a43c9be8634.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-7501513\faac8101-74aa-417c-85d7-86b18167b165.jpg" /> Here, the divergent contributions corresponding to the first term on the right hand side of Equations (6) and (7) are regulated by Λ. The effective quark mass, M, and the effective chemical potential, &#181;, are obtained from solving the following coupled self consistent equations</p><disp-formula id="scirp.40913-formula114709"><label>(9)</label><graphic position="anchor" xlink:href="5-7501513\f19566f0-f304-4a70-abf6-67362dc7a60d.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.40913-formula114710"><label>(10)</label><graphic position="anchor" xlink:href="5-7501513\577fabc7-b73c-458d-92b5-48e80d6d2738.jpg"  xlink:type="simple"/></disp-formula><p>Let us now review the main effects of the repulsive vector interaction in the phase diagram by considering the standard parametrization. <xref ref-type="fig" rid="fig3">Figure 3</xref> shows the situation for G<sub>S</sub> Λ<sup>2</sup> = 2.44, Λ = 587.9 MeV and m<sub>c</sub> = 0 (chiral limit) at G<sub>V </sub>/G<sub>S</sub> = 0, 0.1, and 0.4. As expected the G<sub>V</sub> term has little effect at low chemical potential values where the second order chiral transition dominates since m<sub>c</sub> = 0.</p><p>One also notices that, as G<sub>V</sub> increases, the first order chiral transition line weakens so that the tricritical point occurs at smaller temperatures. It is also clear that for a given temperature the coexistence chemical potential takes place at higher values with increasing G<sub>V</sub>. This scenario is also observed away from the chiral limit <img src="5-7501513\9c124766-7741-4eef-885c-106a2af98fca.jpg" /> except that now the second order transition is replaced by a cross over region and the tricritical point turns into a critical end point. This type of phase diagram where a CP naturally appears at the physical quark mass point is predicted by most model approximations. Now, in order to simulate the lattice results by de Forcrand and Philipsen we first need to obtain a first order phase transition at μ = 0 for low m<sub>c</sub> values so that at vanishing densities our results would be consistent with the lattice results furnished by the Columbia plot [<xref ref-type="bibr" rid="scirp.40913-ref17">17</xref>] .</p><p>Within the NJL this is easily achieved by increasing G<sub>S</sub> [<xref ref-type="bibr" rid="scirp.40913-ref9">9</xref>] so that, at G<sub>V</sub> = 0 and m<sub>c</sub> = 0, the whole phase diagram is dominated by a first order phase transition. <xref ref-type="fig" rid="fig4">Figure 4</xref> shows this situation in the strong coupling regime for different values of G<sub>V</sub> and m<sub>c</sub>. Let us first analyze the case G<sub>V</sub> = 0 by noticing that if one increases m<sub>c</sub> the first order line weakens and turns into a cross over at μ = 0. <xref ref-type="fig" rid="fig5">Figure 5</xref> illustrates the situation in the μ − m<sub>c</sub></p><p>plane showing that, for G<sub>V</sub> = 0, the first order line recedes from the temperature axis as m<sub>c</sub> increases without reproducing the back-bending scenario which would conciliate the de Forcrand and Philipsen results with model predictions. Now, if we turn on the vector interaction, still at m<sub>c</sub> = 0, the weakening of the first order transition happens in a different way so that two segments of first order chiral transitions appear. One of them is the usual one which starts at T = 0 while the other is an unusual first order line which starts at μ = 0 as <xref ref-type="fig" rid="fig4">Figure 4</xref> shows. So, at the expense of considering a strong G<sub>S</sub> and a finite G<sub>V</sub> we have managed to induce the appearance of two tricritical points at vanishing m<sub>c</sub> which, as will be shown in Section 3, leads to the back-bending scenario.</p></sec><sec id="s2_2"><title>2.2. Thermodynamical Potential at Vanishing G<sub>V</sub> with Finite N<sub>c</sub> Contributions</title><p>The basic idea of the OPT method is to deform the original lagrangian density by adding a quadratic term like <img src="5-7501513\78eda869-243f-42b3-a873-70aca98b272a.jpg" /> to the original lagrangian density as well as by multiplying all coupling constants by δ [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] . The new parameter δ is just a bookkeeping label and η represents an arbitrary mass parameter. Perturbative calculations are then performed in powers of the dummy parameter δ which is formally treated as small and set to the original value, δ = 1, at the end<sup>1</sup>.</p><p>Therefore, the fermionic propagator is dressed by η which may also be viewed as an infrared regulator in the case of massless theories. After a physical quantity, such as the thermodynamical potential (Ω), is evaluated to the k-order and δ set to the unity only a residual η dependence remains. Then, optimal nonperturbative results can be obtained by requiring that Ω(k) (η) be evaluated where it is less sensitive to variations of the arbitrary mass parameter. This requirement translates into the criterion known as the Principle of Minimal Sensitivity (PMS) [<xref ref-type="bibr" rid="scirp.40913-ref18">18</xref>]</p><disp-formula id="scirp.40913-formula114711"><label>(11)</label><graphic position="anchor" xlink:href="5-7501513\0773bac6-f39f-4a72-bb87-8b37d1520948.jpg"  xlink:type="simple"/></disp-formula><p>In general, the solution to this equation implies in self consistent relations generating a nonperturbative coupling dependence. In most cases nonperturbative <img src="5-7501513\846fc73b-12d8-4f37-9f1e-e3309d1c3bd1.jpg" /> corrections appear already at the first nontrivial order while the large-N<sub>c</sub> (or MFA) results can be recovered at any time simply by considering N<sub>c</sub> → ∞. Finally, note that the OPT has the same spirit as the Hartree and the Hartree-Fock approximation in which one also adds and subtracts a mass term. However, within these two traditional approximations the topology of the dressing is fixed from the start: direct (tadpole) terms for Hartree and direct plus exchange terms for Hartree-Fock. On the other hand, within the OPT, the dressed mass term <img src="5-7501513\405b3fa2-ed74-43b3-a4db-8760139ca316.jpg" /> acquires characteristics which change order by order progressively incorporating direct, exchange, vertex corrections, etc, effects. The differences between these three different methods have been recently discussed in [<xref ref-type="bibr" rid="scirp.40913-ref14">14</xref>] . To implement the OPT within the NJL model at G<sub>V</sub> = 0 one follows the prescription used in [<xref ref-type="bibr" rid="scirp.40913-ref13">13</xref>] to write</p><disp-formula id="scirp.40913-formula114712"><label>(12)</label><graphic position="anchor" xlink:href="5-7501513\e53eb1b6-45d4-4050-a4b0-d8156c376cc5.jpg"  xlink:type="simple"/></disp-formula><p>Then, the order-δ thermodynamical potential can be written as (see [<xref ref-type="bibr" rid="scirp.40913-ref13">13</xref>] for technical details)</p><disp-formula id="scirp.40913-formula114713"><label>(13)</label><graphic position="anchor" xlink:href="5-7501513\993cb856-4cd8-4140-9514-8004d0174be5.jpg"  xlink:type="simple"/></disp-formula><p>where now all the integrals <img src="5-7501513\7f75d5a5-13d7-4743-8a2f-1d3964a9f8f5.jpg" /> defining the quantities ω<sub>FG</sub>, ρ<sub>s</sub> , and ρ<sub>q</sub> are redefined as<img src="5-7501513\5837b168-750f-4490-a797-25d370d60dfc.jpg" />. Then, for each pair of <img src="5-7501513\48dd1c6e-4b87-4f73-8957-1b1cc432ea52.jpg" /> values the optimum mass parameter, <img src="5-7501513\41638d01-e0ad-4685-a957-f5434fef1600.jpg" />, can be obtained by solving the PMS equation given by [<xref ref-type="bibr" rid="scirp.40913-ref13">13</xref>]</p><disp-formula id="scirp.40913-formula114714"><label>(14)</label><graphic position="anchor" xlink:href="5-7501513\c825b14c-b15f-400d-87b0-6f6363d5b9aa.jpg"  xlink:type="simple"/></disp-formula><p>Note that when N<sub>c</sub> → ∞ the PMS optimization procedure sets <img src="5-7501513\94f1d1a7-6207-4201-a720-930b3bdfb849.jpg" />= −2G<sub>S</sub>ρ<sub>s</sub> exactly reproducing the large-N<sub>c</sub> result (for the standard NJL model) with no ρ<sub>q</sub> dependence. By comparing the OPT thermodynamical potential given by Equation (13) with its large-N<sub>c</sub> counterpart given by Equation (2) one notices that the OPT induces a finite N<sub>c</sub> correction of the form <img src="5-7501513\181daf08-fe28-42cf-8b11-c13cf6128bfc.jpg" /> while, as discussed in [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] , the G<sub>V</sub> term gives a net contribution of the form G<sub>V</sub> ρ<sub>q</sub><sup>2</sup>. Then, one could expect that the two different model approximations given by the OPT (at G<sub>V</sub> = 0) and the large-N<sub>c</sub> approximation (at G<sub>V</sub> ≠ 0) lead to the same qualitative picture of the phase diagram. A recent comparison performed with one flavor at vanishing temperature in [<xref ref-type="bibr" rid="scirp.40913-ref14">14</xref>] showed that this is indeed the case.</p><p>Here, we are now in position to extend that comparison to the more realistic two flavor case at finite temperatures.</p></sec></sec><sec id="s3"><title>3. Comparing the OPT at G<sub>V</sub> = 0 with the Large-N<sub>c</sub> Approximation at G<sub>V</sub> = 0</title><p>Let us now compare the results furnished by the two approximations for the NJL model at high G<sub>S</sub>. <xref ref-type="fig" rid="fig6">Figure 6</xref> shows the T − μ phase diagram when chiral symmetry is weakly broken<img src="5-7501513\514e43d0-0688-4431-9375-f35a8fe67ad5.jpg" />. This figure also shows the large-N<sub>c</sub> result for G<sub>V </sub>= 0 which predicts a first order transition taking place in the whole plane. At the same time the OPT with its <img src="5-7501513\39cac43d-6950-42be-b756-edb0cd51b930.jpg" /> contribution and the large-N<sub>c</sub> at G<sub>V</sub> ≠ 0 weaken that line at intermediate chemical potential values so that two critical points appear in this case of small current mass as expected from the discussion related to <xref ref-type="fig" rid="fig2">Figure 2</xref>. Then, by varying the m<sub>c</sub> values towards the physical one (m<sub>phys</sub>) one can map the T − μ diagram into the μ − m<sub>c</sub> plane as shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>. This figure clearly shows that both approximations considered here manage to produce the back-bend-</p><p>ing of the critical line so that the CP will be recovered at m<sub>c</sub> = m<sub>phys</sub> even if initially (at low values of μ) the line bends in such a way which is reminiscent of the “exotic” scenario displayed by the right panel of <xref ref-type="fig" rid="fig1">Figure 1</xref>. The physical nature and even the critical exponents of the two different critical points which occur at small m<sub>c</sub> have been discussed in great detail in [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] . From our results it is clear that as m<sub>c</sub> → m<sub>phys</sub> the unusual first order line disappears and only the usual “liquid-gas” type of first order line survives in accordance with most model predictions.</p></sec><sec id="s4"><title>4. Conclusions</title><p>We have considered the two flavor NJL model in the strong scalar coupling regime (G<sub>S</sub>Λ<sup>2</sup> @ 4) in order to compare two distinct model approximations. The first is the traditional large-N<sub>c</sub> approximation which was applied by explicitly considering a finite repulsive vector interaction (proportional to G<sub>V</sub>) which was introduced at the classical (tree) level. The second is the alternative OPT method which was applied to the standard version of the NJL model<img src="5-7501513\a7c5b476-1696-46fa-8f3b-d370fd3c40d2.jpg" />.</p><p>Our first step towards the simulation of the backbending behavior was to tune G<sub>S</sub> at G<sub>V</sub> = 0 so that the large-N<sub>c</sub> approximation predicts that the first order transition line, which usually starts at T = 0, will touch the T axis at μ = 0 for very small m<sub>c</sub> values.</p><p>For mass values closer to the physical ones, this approximation recovers the expected cross over behavior at small μ with the appearance of a single critical point at intermediate chemical potentials. Next, we have shown that by considering finite values for G<sub>V</sub> at <img src="5-7501513\aeb49a6d-9a85-4379-8f61-237ef7c26546.jpg" /> this single first order transition line splits into two lines in the T − μ plane. One of them is similar to the usual “liquid-gas” line which starts at T = 0 and ends at intermediate temperature values. The other one, which has a more “chiral” behavior according to the analysis of [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] , is located at the high temperature region and disappears as m<sub>c</sub> approaches m<sub>phys</sub> from below. In this way, we were able to induce the back-bending behavior for two flavors in a manner analogous to the one adopted in [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] for the three flavor case. The OPT results for this strong coupling and small regime obtained in [<xref ref-type="bibr" rid="scirp.40913-ref7">7</xref>] were then reviewed so that a numerical comparison could be performed. At the first non trivial order, this approximation includes one and two loop terms which would belong to the <img src="5-7501513\c5215bce-5928-4f47-9ed1-b9da2a490000.jpg" /> and <img src="5-7501513\8b907432-c011-45e4-891c-f3ec7a81cddd.jpg" /> in the usual <img src="5-7501513\cb81db8d-b6e2-495e-ac33-38b4fce43961.jpg" /> type of expansion. In particular, the two loop terms generate a negative contribution to the pressure given by <img src="5-7501513\ed0740bf-701f-4dab-939f-254216f883cc.jpg" />, where ρ<sub>q</sub> represents the fermionic density. This term is similar to the net −G<sub>V </sub>ρ<sub>q</sub><sup>2</sup> contribution considered at large-N<sub>c</sub> [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] . Within the OPT the <img src="5-7501513\b0e1fa91-f20e-4d10-bc09-52cc674477c9.jpg" /> suppressed vector term competes with its scalar counterpart, ρ<sub>s</sub>, weakening the first order line at intermediate values of μ and enhancing the appearance of two critical points in the T − μ plane for m<sub>c</sub> values which are smaller than the physical ones. Finally by scanning the values of m<sub>c</sub>, we have mapped the T − μ phase diagram into the μ − m<sub>c</sub> plane observing that, for strong couplings, the large-N<sub>c</sub> approximation, at finite G<sub>V</sub><sub> </sub>, and the OPT, at vanishing G<sub>V</sub> , predict that the first order transition region shrinks for low values of μ as observed in the lattice simulations of [<xref ref-type="bibr" rid="scirp.40913-ref1">1</xref>]. But then, at intermediate chemical potentials, the vector terms −G<sub>V </sub>ρ<sub>q</sub><sup>2</sup> (large-N<sub>c</sub>) and <img src="5-7501513\1e348c76-c578-47d2-ae75-a1a2acdb682f.jpg" /> (OPT) change the first order phase transition region into a cross over region. Finally, at higher chemical potentials, the first order transition region reappears and then expands as μ is increased. So, our results suggest that even if an initial shrinkage of the first order region is confirmed by lattice simulations, it does not necessary rule out the existence of the CP which is expected to occur at intermediate chemical potentials for physical quark masses. In this case, a back-bending will be observed on the μ − m<sub>c</sub> plane outlining the importance of a repulsive vector contribution in agreement with [<xref ref-type="bibr" rid="scirp.40913-ref4">4</xref>] . Our comparison allows us to conclude that similar qualitative results will be obtained either by explicitly considering such a contribution at the classical level as in the large-N<sub>c</sub> case or by radiatively generating it by going beyond the mean field level. Within the NJL model, the advantage of the second procedure, which can easily be implemented within the OPT, is that it does not require the fixing of G<sub>V</sub> which is a drawback of the first procedure. The results obtained in the present application support those obtained in [<xref ref-type="bibr" rid="scirp.40913-ref14">14</xref>] , for the simpler abelian NJL model at vanishing temperature, showing the robustness of the OPT method. Finally, note that at these non standard high coupling values our results are to be taken only as qualitative predictions.</p></sec><sec id="s5"><title>5. 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