Research Article  Open Access
WeiShu Hou, "Bootstrap Dynamical Symmetry Breaking", Advances in High Energy Physics, vol. 2013, Article ID 650617, 19 pages, 2013. https://doi.org/10.1155/2013/650617
Bootstrap Dynamical Symmetry Breaking
Abstract
Despite the emergence of a 125 GeV Higgslike particle at the LHC, we explore the possibility of dynamical electroweak symmetry breaking by strong Yukawa coupling of very heavy new chiral quarks . Taking the 125 GeV object to be a dilaton with suppressed couplings, we note that the Goldstone bosons exist as longitudinal modes of the weak bosons and would couple to with Yukawa coupling . With GeV from LHC, the strong could lead to deeply bound states. We postulate that the leading “collapsed state,” the colorsinglet (heavy) isotriplet, pseudoscalar meson , is itself, and a gap equation without Higgs is constructed. Dynamical symmetry breaking is affected via strong , generating while selfconsistently justifying treating as massless in the loop, hence, “bootstrap,” Solving such a gap equation, we find that should be several TeV, or , and would become much heavier if there is a light Higgs boson. For such heavy chiral quarks, we find analogy with the system, by which we conjecture the possible annihilation phenomena of with high multiplicity, the search of which might be aided by Yukawabound resonances.
1. Introduction and Motivation
The field of particle physics is in a state of both jubilation and anxiety. On one hand, the longawaited Higgs boson seems to have finally emerged [1, 2] at ~125 GeV at the LHC, where a hint appeared already with 2011 data [3, 4]. The case has been further strengthened with more data added by end of 2012, and the final results for the 78 TeV run would be revealed by the Moriond meetings in 2013. On the other hand, there appears to be no New Physics below the TeV scale, and one is worried what really stabilizes the Higgs mass at 125 GeV.
As much as the existence of a 125 GeV boson is beyond doubt, we note that it is not yet experimentally established that it is the Standard Model (SM) Higgs boson. In part because of the enhancement in mode—for both ATLAS and CMS, and for both 7 and 8 TeV data—and also because the subdominant production channels are not yet experimentally firm, the 125 GeV object could still be a dilaton [5–7]. The dilaton couples like a Higgs boson, but with couplings suppressed by , where is the observed vacuum expectation value (v.e.v.) of electroweak symmetry breaking (EWSB), and is the “dilaton decay constant” that is related to scaleinvariance violation. The dilaton couplings to and , however, are determined by the trace anomaly of the energymomentum tensor and would depend on UV details. Keeping and effective and couplings free, it is found [6] that a “dilaton” interpretation is as consistent as an SMHiggs. To reject the dilaton, one has to establish the subdominant vector boson fusion (VBF) and Higgsstrahlung, or associated production (VH) processes at the expected SM level. Judging from the results available at the end of 2012, it seems [8] that the issue would have to await the restart of the LHC at 13 TeV.
Regardless of whether the 125 GeV object is the SM Higgs boson or a dilaton, the Higgs mechanism is an experimental fact. That is, the electroweak (EW) gauge symmetry is experimentally established, while the gauge bosons, as well as the chirally charged fermions, are all found to be massive, in apparent violation of the gauge symmetry. Thus, the Goldstone particle of EWSB gets “eaten” by the EW gauge bosons, which become massive (the Meissner effect), as has been experimentally established since 30 years. The v.e.v. is simply related to the venerable Fermi constant .
With both quarks and gauge bosons massive, a heuristic argument was used to demonstrate [9] that, starting from the lefthanded vector gauge coupling, the longitudinal component of the EW gauge boson, that is, equivalently the Goldstone boson , couples to quarks by the SM Yukawa coupling, with both left and righthanded components. Thus, Yukawa couplings are experimentally established. Furthermore [9], much of flavor physics and violation (CPV) studies probe the effects of Yukawa couplings, providing ample and highly nontrivial support for their “complex” existence.
A natural question to ask is as follows: given three quark generations already, could there be a fourth copy? Does it carry its own raison d’être? It is not our purpose to discuss in detail the issues, merits, and demerits regarding this possible fourth generation (4G), which we refer to [10]. At face value, we admit that the observed 125 GeV new boson would pose a difficulty. The main issue is not so much the existence of the Higgs boson, but one as light as 125 GeV. The gluongluon fusion production, through the top loop in SM, is now augmented by 4G quarks and in the loop, leading to an enhancement of order in production crosssection, which does not seem reflected by data. In fact, searches [11] assuming this enhancement factor rule out a Higgs boson in the full mass range up to 600 GeV. We are reminded, however, that by simply extending from generations, the effective CPV increases [12] by a thousandtrillionfold or more and may provide enough CPV to satisfy the Sakharov conditions for baryogenesis. Given that the threegeneration KobayashiMaskawa model [13] falls far short of the needed CPV, Nature might use such an enhancement factor. Furthermore, before one rules out the dilaton possibility, the premise for the order of magnitude enhancement in production may not stand.
Fourth generation and quarks have been pursued vigorously at the LHC, as it should be done for a hadron collider, independent of the Higgs situation. The current bound [14–20] is where stands for a chiral quark doublet, in which the limit is from both and search. We shall assume “heavy isospin” symmetry, , and treat the doublet as degenerate, which can be viewed as part of the custodial SU symmetry. What is important is that the current bound is already above the nominal perturbative partial wave unitarity bound (UB) of 550 GeV [21]. The Yukawa coupling (where ) has already entered the strong coupling regime; .
With the ever increasing bound on , the fourth generation may well not exist. But being beyond UB, a new question is as follows: could the strong Yukawa coupling of generate [22] EWSB itself? This is an intriguing conjecture and provides a second reason for having a fourth generation. Along this line, a gap equation, given symbolically in Figure 1, was constructed [9] without ever invoking the Higgs doublet, that is, the Higgs boson field of SM.
The logic or philosophy went as follows. The Goldstone boson is viewed as a tightly bound state, bound by the Yukawa coupling itself. Guided by a BetheSalpeter equation study [23], strong Yukawa binding could lead to state collapse; that is, the bound state turns tachyonic, which is taken as suggestive of triggering EWSB itself. For further elucidation, see [24]. Reference [9] went one step further to postulate that the leading collapsed state, the colorsinglet isosinglet pseudoscalar meson, , is the Goldstone boson itself. With no New Physics in sight at the LHC, not even the heavy chiral quark itself, the loop momentum integration runs up to roughly (when the Goldstone boson ceases to exist), without the need to add any further effects (in the ladder approximation of truncating corrections to propagation and vertex). This is therefore a “bootstrap” gap equation, in that the strong Yukawa coupling itself is the source of EWSB, or mass generation for quark , which simultaneously justifies keeping the Goldstone in the loop (the 125 GeV object is assumed to be the dilaton). The existence of a large Yukawa coupling is used as input, without a theory for itself. There is no attempt at UV completion.
It is important then to investigate whether one could find a solution to such a gap equation. If so, we would have demonstrated the case for dynamical symmetry breaking (DSB) and the potential riches that could follow. This paper offers a comprehensive elucidation of the line of thought from the aforementioned, through the demonstration of DSB, and linking the need of 23 TeV quarks to the possible new phenomenon of production, the search of which could be aided by Yukawa resonances.
In Section 2, we trace the arguments that set up the bootstrap gap equation, including the postulate of the Goldstone boson as a “collapsed state.” In Section 3, we formulate this gap equation more clearly, and demonstrate that numerical solution does exist [8]. A similar gap equation was formulated by Hung and Xiong [25], where in Figure 1 is replaced by a massless Higgs doublet field. We will compare and offer a critique. Our numerical solution [8] suggests to be in the 23 TeV range, corresponding to . Even for lower than this range, one may ask whether the usual assumption of followed by free decay would hold, as assumed so far in direct searches [14–20]. The large Yukawa coupling now resembles the coupling in strength; to our surprise, we find . We tap into the known phenomena and conjecture that , with multiplicity ~6–12, and with a characteristic temperature of order that is to be measured. This is discussed in Section 4. We end with further discussions and offer a conclusion in Section 5.
2. A Gap Equation without Higgs
My own interest in the 4th generation was revitalized by a hint of possible New Physics in electroweak penguin contributions to direct CPV in decay (e.g., see, the account given in [12]). In between 2007 and 2008, my interest turned to direct search for and at the LHC with the CMS experiment. Although initially I wished for GeV for sake of the rich phenomenology [26, 27], I found the link [22] of strong Yukawa coupling with EWSB rather intriguing. As the direct search limits on and rose, I began to find the usual Higgs mechanism via an elementary Higgs doublet more and more problematic. Having just in the Lagrangian lacked dynamics (it is only a description), while Nature seems to be saying something through the absence of elementary scalars in QED and QCD, where the dynamics are better understood than EWSB. Furthermore, most problems such as the hierarchy problem arose by treating the Higgs doublet field as elementary.
The following is how curiosity led the way from a flavor/CPV entry into dynamical EWSB, without invoking the existence of an elementary Higgs doublet field.
2.1. Yukawa Coupling from Gauge Coupling
Holding the SMHiggs interpretation of the 125 GeV particle observed [1, 2] at LHC as still suspect, let us recall the firm facts from experiment.
First, we know [28] that all observed quarks and charged leptons are pointlike to smaller than m, and they are governed by the gauge dynamics. Chromodynamics would not be our concern, but it is important to emphasize that, unlike the 1970s and early 1980s, the chiral gauge dynamics is now experimentally established. We know that quarks and leptons come in lefthanded weak doublets and righthanded singlets, and for each given electric charge, they carry different hypercharge .
Second, the weak bosons are found [28] to be massive; , where is the measured weak coupling, and the vacuum expectation value. Hence, spontaneous breaking of symmetry (SSB) is also experimentally established.
Third, all fermions are observed [28] to be massive. These masses also manifest EWSB, since they link left and righthanded fermions of the same electric charge, but different and charges. We shall not invoke the elementary Higgs boson for mass generation, as this is the question we explore, and because the dilaton possibility has to be ruled out by experiment.
At this point, we need to acknowledge the important theoretical achievement of renormalizability [29] of nonAbelian gauge theories, which allowed theoryexperiment correspondence down to per mille level precision, especially for the extensive work [28] done at the LEP, SLC, as well as TeVatron colliders. The proof of renormalizability is based on Ward identities, hence, [30] unaffected by SSB; that is, the underlying symmetry properties are not affected. From this, we now demonstrate [9, 31] the existence of Yukawa couplings as experimental fact.
With proof of renormalizability, we choose the physical unitary gauge; hence, there are no wouldbe Goldstone bosons (or unphysical scalars), only massive gauge bosons (strictly speaking, only the onshell matrix is finite in gauge, we thank T. Kugo for the comment and take it as a limiting case of the gauge for sake of illustration). Longitudinal boson (the wouldbe Goldstone bosons that got “eaten”) propagation is via the part of the boson propagator. If we take a factor and contract with a charged current, as illustrated in Figure 2, simple manipulations give (dropping for convenience) where we have inferred as the effective , or Goldstone boson coupling to quarks, which is nothing but the familiar Yukawa coupling. We have used the equation of motion, that is, the Dirac equation, on and quarks in the second step of (2), but this is justified since we exist in the broken phase for the real world, and we know experimentally that all quarks are massive.
From Figure 2 and equations (2) and (3), we see that from the experimentally wellestablished lefthanded gauge coupling, the Goldstone boson couples via the usual Yukawa coupling. The Goldstone bosons of EWSB pair with the transverse gauge boson modes to constitute a massive gauge boson, the Meissner effect, but the important point is that we have not introduced a physical Higgs boson in any step. Unlike the Higgs boson, SSB of electroweak symmetry is an experimentally established fact. The Goldstone bosons couple with Yukawa couplings proportional to fermion mass, independent of whether it arises from an elementary Higgs doublet.
We have kept a factor in Figure 2. Recall that the KobayashiMaskawa (KM) formalism [13] for quark mixing deals with massive quarks, or equivalently the existence of Yukawa matrices, and the argument remains exactly the same. Vast amount of flavor and violation (CPV) data overwhelmingly supports [28] the 3 generation KM picture. For example, the unique CPV phase with 3 quark generations can so far explain all observed CPV phenomena. These facts further attest to the existence of Yukawa couplings from their dynamical effects but again do not provide any evidence for the existence of the SM Higgs boson.
2.2. A Postulate: Collapse of Yukawa Bound State
Based on experimental facts and the renormalizability of electroweak theory, we have “derived” Yukawa couplings from purely lefthanded gauge couplings in the previous section, without invoking an explicit Higgs sector, at least not at the empirical, heuristic level. We turn now to a more hypothetical situation: could there be more chiral generations? Since we already have three, the possibility that there exists a fourth generation of quarks should not be dropped in a cavalier way. We note again that increasing to 4 generations, one may have sufficient amount of CPV for baryogenesis [12] from the KM mechanism. There has also been some resurgent recent interest [10, 14–20]. As argued in the Introduction, although the spirit may have been dampened by the 125 GeV Higgslike object, one should press on with the direct search.
What we do know is that the and quarks should be suitably degenerate to satisfy electroweak constraints on the and variables [32]. A “heavy isospin” is in accordance with the custodial SU symmetry.
2.2.1. Relativistic Expansion versus BetheSalpeter Equation
With GeV [14–20], is already 4 times stronger than the top quark, hence, stronger than all gauge couplings. There have been two complementary studies of strong Yukawa bound states. The first approach is along traditional lines of relativistic expansion [33]. Ignoring all gauge couplings except QCD, and taking the heavy isospin limit, with representing the 4th generation quark doublet, and the triplet of Goldstone bosons, the  and channel Goldstone exchange diagrams are depicted in Figure 3, with corresponding diagrams for as well as exchange ([33] did not put in channel gluon exchange).
The heavy mesons form isosinglets and isotriplets and can be color singlet or octet. We borrow the notation from hadrons and call these states , , , , and , , , , respectively. Reference [33] used a variational approach, with radius as parameter. It was found that, for color singlet , for below 400 (540) GeV, but above which suddenly precipitates towards tiny values. For , the radius mildly decreases (increases) from 1, with trend reversed for binding energy; hence, it remains QCDbound.
To understand this, note that the channel Goldstone exchange for is repulsive, while the channel Goldstone exchange, contributing only to , is also repulsive. However, the sudden drop in and radii is due to the trial wave function sensing suddenly a lower energy at tiny radius due to channel Goldstone exchange; the strong Yukawa coupling has wrested control of binding from the Coulombic QCD potential. QCD binding energy is only a couple of GeV, but the sudden drop in radius leads to a sharp rise in binding energy, hence, a kink. One finds that the relativistic expansion fails just when it starts to get interesting. For color octet states, QCD is repulsive; so, does not bind. In [33], the and states are degenerate, with sudden shrinking of radius occurring around 530 GeV, but the channel QCD effect, left out in [33], should push the upwards; the state does not shrink until later.
Given that the relativistic expansion breaks down, a truly relativistic approach is needed. Such a study, based on a BetheSalpeter (BS) equation [23], was pursued around the time of demise of the SSC, for very heavy chiral quark doublets. The BS equation is a ladder sum of  and channel diagrams of Figure 3, where the pair forms a heavy meson bound state. While the ladder sum of channel diagrams is intuitive, a problem emerges for the channel, which contributes only to , , and (same quantum numbers as , , and , resp.). Rather than a triangle loop, the channel loop appears like a selfenergy, hence, potentially divergent, while the momentum carried by the exchanged boson is the bound state mass itself. One could not formally turn the integral equation into an eigenvalue problem. This was resolved in [23] by a subtraction at fixed external momentum, which in effect eliminates all channel diagrams. Reference [23] then solved the BS equation numerically using several different approximations, which, in addition to the approximate nature of the BS equation itself, illustrates the uncertainties. Still, unlike [33], the bound state masses drop smoothly below as increases, showing no kink, which is an improvement from a relativistic expansion. However, a generic feature is collapse; bound state masses tend to drop sharply to zero at some high and would naively turn tachyonic.
2.2.2. Postulate for Leading Collapsed State
Here, we do not pursue the more conservative phenomenology for precollapse Yukawa couplings as in [24] but wish to address more fundamental issues. Although the de facto channel subtraction made by [23] appeared reasonable on formal grounds, the contrast with the relativistic expansion is striking; the Goldstone exchange in channel led to a specific repulsion [33] for heavy mesons, disallowing it to shrink suddenly like the otherwise analogous . But after subtracting the channel, the becomes [23] the most attractive channel (MAC), more so than . Together with the tendency towards collapse for large enough (equivalently ), this means that the meson would be the first to drop to zero and turn tachyonic. That this occurs for the channel that experiences repulsion when is far lower than collapse values (à la which has no channel effect) seems paradoxical. Does this falsify the whole approach, or else what light does this shed? And how is it related to channel subtraction?
With experimental bounds [14–20] for 4th generation quarks entering the region of deep(er) binding, we offer a selfconsistent view that may seem radical. Clearly, around and below 500 GeV mass, or TeV, there could still be some repulsion due to exchange in channel. But since we did not introduce any elementary Higgs doublet, the Goldstone boson should perhaps be viewed as a bound state. Hence, we Postulate (). Collapse is a precursor to dynamical EWSB, and the first mode to collapse becomes the Goldstone mode.
Although the full validity of the BS equation may be questioned, it is known [34] that “the appearance of a tachyonic bound state leads to instability of the vacuum,” which is “resolved by condensation into the tachyonic mode.” Our postulate removes the equation for selfconsistently (there is another aspect on the selfconsistency of this subtraction/postulate, if one did not remove the equation by invoking this subtraction, the leading collapse state of strong Yukawa coupling would be the , condensation in this channel would break Lorentz invariance) and provides some understanding of the channel subtraction; a boson carrying would no longer be a bound Goldstone boson in channel. Without an elementary Higgs boson, there is no channel subtraction, while for heavy enough (so has turned Goldstone), one can treat QCD effects as a correction, after solving the bound state problem, without need of subtracting channel exchange. The selfconsistent MAC behavior of the channel seems like a reasonable outcome of the Goldstone dynamics, as implied by the gauge dynamics.
It may now appear that EWSB is some kind of a “bootstrap” from “massive chiral quarks” with large Yukawa coupling as seen in broken phase.
2.3. A Bootstrap Gap Equation without Higgs
Motivated by the previous heuristic discussion, we construct a gap equation for the dynamical generation of heavy quark mass without invoking the Higgs boson.
For a long time, as limit rose, I focused on breaching the UB, which the experimental pursuit would not be concerned about. Although UB violation (UBV) occurs at far higher energy, once the experimental limits breach the bound, some form of strong interactions would take over. I asked myself how UBV might be amended by Nature. The study of Yukawa bound states [24] arose from this pursuit, but did not shed sufficient light on the issue, except approaching the abyss of state “collapse”, as described earlier.
A mindset change occurred when one connected two of the or lines in Figure 3. One gets the selfenergy for by exchange and readily arrives at the gap equation [9] as depicted in Figure 1. If quark mass , represented by the cross , could be nonzero, then one has dynamical chiral symmetry breaking, which is equivalent to EWSB! Both and are treated as massless at the diagrammatic level, since the gap equation is summing over all possible momenta carried by as it mediates—dominates— scattering. But if reaches , there would no longer be a Goldstone boson (assuming is a bound state), or it would be resolved in the channel. Thus, the summation over should not exceed at the heuristic level. The whole picture is heuristic, but realistic in the experimental sense, since the gap equation integrates over a large momentum range of , where we have no other New Physics that enter, as indicated by LHC data.
Such a gap equation was constructed recently from a different, and in our view more ad hoc, theoretical argument. In [25], an elementary Higgs doublet is assumed together with a 4th generation. Motivated by their earlier study [35, 36], where some UV fixed point (UVFP) behavior was conjectured, these authors pursued dynamical EWSB via a SchwingerDyson equation that is rather similar to our Figure 1. However, perhaps in anticipation of the UVFP that might develop at high energy [35, 36], they put in by hand a massless Higgs doublet, hence, a scale invariant theory to boot. It is the massless Higgs doublet that runs in the loop, replacing our Goldstone boson . The massless nature of the Higgs doublet appears ad hoc, and the paper defers the discussion of the physical Higgs spectrum for a future work.
In contrast, our Goldstone boson , identified as the collapsed state as it turns tachyonic, is strictly massless in the broken phase. In the gap equation of Figure 1, we speculate that the loop momentum should be cut off around , rather than some “cutoff” scale . In so doing, we bypass all issues of triviality that arise from having approaching . What happens at scales above is to be studied by experiment.
Here, we remark that the first, elementary Higgs of [25], and are our bound state Goldstone bosons, and indeed we should have a like massive broad bound state [24] that could mimic the heavy Higgs boson. Their second Higgs doublet, in the form of and bound states, would be excitations above the and for us, likely rather broad. We think that their claimed third doublet, that of bound and , may not be bound at all, as their Yukawa couplings may not be large enough.
The gap equation illustrated in Figure 1 actually links to a vast literature on strongly coupled, scaleinvariant QED. It is known that such a theory could have spontaneous chiral symmetry breaking when couplings are strong enough. We turn to our numerical study [8] in the next section, where we also offer our critique of [25].
Although our line of thought may seem constructed, we have developed a selfconsistent picture where EWSB from large Yukawa coupling may be realized with some confidence—all without assuming an elementary Higgs boson. We have not yet really touched on the meson, which would be the heavy Higgs boson. However, our scenario is to have Goldstone bosons as strongly (and tightly) bound “Cooper pairs” of very heavy quarks, which may please Nambu. For the 125 GeV Higgslike object, the inherent scaleinvariant nature of our gap equation allows the possibility of a dilaton interpretation, as we will discuss later.
3. Solving Bootstrap Gap Equation
The question now is whether the symbolic gap equation of Figure 1 affords actual solutions. Towards finding a solution, in this section, we briefly review the NambuJonaLasinio model, where one sets up a gap equation with its wellknown solution. We then turn to the socalled strongly coupled scaleinvariant QED, which is closer to our gap equation. By recounting some major steps, we also set up our notation for later usage. We find a coupled set of integral equations, which is more complicated than strong QED in Landau gauge. But a numerical solution is found [8], with , where we compare and contrast with [25].
3.1. NJL Model: Independent SelfEnergy
The NambuJonaLasinio model [37] is the earliest, explicit model of DSB, where the breaking of global chiral symmetry leads to generation of nucleon mass, and the pion as a (pseudo) Goldstone boson [38–40]. (Strictly speaking, the Goldstone boson should really be called the NambuGoldstone (NG) boson, since [38] predated [39]. But for sake of notation, and because of more common usage, we shall use and Goldstone boson throughout our paper).
The model is depicted in Figure 4, where a fourfermion interaction is introduced (the blob on the righthand side). The nucleon mass, represented by a cross, is selfconsistently generated. One easily finds the gap equation where here is the fourfermi coupling and is the cutoff. Since on both sides factor out, one has which admits a solution for , with
To understand what is happening, one can iterate the cross of the lefthand side of Figure 4 on the righthand side and see that it constitutes an infinite number of diagrams. This effectively puts the original selfenergy diagram into the denominator. In the end, one trades the parameters and for the physical and the pionnucleon coupling. At the more refined level and using the quark language, one can show further that the emergent Goldstone boson, the pion, is in fact a ladder sum of the quarklevel fourfermi interaction.
We will return at the end to discuss the similarity and differences of the NJL model with our gap equation.
3.2. Strong QED: Dependent SelfEnergy
We note that the selfenergy bubble of Figure 4 does not depend on external momentum , and so at the superficial level, Figure 4 is quite different from Figure 1. We now turn to QED, where there is much closer similarity.
The general gap equation for QED [41] can be written in the form of the SchwingerDyson (SD) equation where is the electron selfenergy with the (full) electron propagator, is the (full) photon propagator, and is the full vertex.
3.2.1. Ladder Approximation
Truncating the exact, full vertex and photon propagator by the approximation called the ladder (or rainbow) approximation, but retaining the electron selfenergy, the gap equation becomes with now given in (9), and we have set , that is, massless QED at Lagrangian level. Pictorially, this is represented as in Figure 5, where we note that, compared with the fourfermion coupling of the NJL model depicted in Figure 4, the external momentum now flows into the selfenergy loop. The question now is whether chiral symmetry can be dynamically broken, that a nontrivial solution to the selfenergy could be generated at some strong coupling ?
We define the electron propagator as [41] where the term corresponds to wave function (w.f.) renormalization related to the usual factor. A finite pole of the propagator, , would give the dynamical effective mass. Our aim is therefore solving and from the gap equation of (10). Inserting (9) and after some algebra, one finds
Simplification can be achieved in the Landau gauge, , where one finds . Since relates to w.f. renormalization, it satisfies the WardTakahashi identity even under the ladder approximation. The gap equation is simplified to a single equation After Wick rotation, and using one obtains where is the Euclidean momentum squared, and , are the ultraviolet (UV) and infrared (IR) cutoffs, respectively.
The integral equation can be changed to a differential equation by noting One obtains the differential equation together with the IR and UV boundary conditions (B.C.) If IR cutoff is 0, the B.C. for IR should be replaced by at .
3.2.2. Solution in Landau Gauge
The coupled integral equations are simplified and put into a differential equation with B.C. In order to study qualitative features, let us first find an approximate solution. For a special range for the IR cutoff, let us take ; then, (17) is simplified to Inserting , the characteristic equation is with discriminant ; hence, the behavior is different for and , where . The analytical solution under the approximation is given as and the boundary conditions can be written as The determinant must vanish for nontrivial ; hence, To satisfy this condition, is needed, and for given , takes on discontinuous values One sees that for , the nominal “continuum limit.” For , the only solution that satisfies the B.C. is the trivial .
The approximate solution for small IR cutoff can now be obtained by replacing (constant) for small . The differential equation becomes where is a hypergeometric function. Namely, where and is a hypergeometric function. Checking the asymptotic behavior for , the power behavior for cannot satisfy the UV boundary condition.
The gap equation has a nontrivial or oscillatory solution for , where the critical coupling is for QED. The dynamical effective mass is obtained by solving . Note that the pole of the propagator should be given in the timelike region; so, one has to make analytical continuation in order to obtain a physical mass, which can be done smoothly for .
An issue arises in that the dynamical mass is proportional to the UV cutoff . For to be physical, however, it should not depend on . Miransky suggested [42] that as ; that is, is a nontrivial UV fixed point. A related issue, which we would not go into, is whether there would be a dilaton associated with breaking of scale invariance [43, 44]. (These two are also the two best references for gauged NJL model).
3.3. Bootstrap Gap Equation for EWSB
Our recapitulation of strong QED is for the purpose of setting up our approach for solving the bootstrap gap equation [9] with large empirical Yukawa coupling, where we will continue to follow the FukudaKugo approach.
In Landau gauge (), the propagations of (wouldbe) Goldstone modes and gauge bosons are properly separated, and the gap equation becomes equivalent to our discussion if one takes the limit for the gauge coupling. The Goldstone bosons and couple to fermions with the familiar Yukawa couplings, which we have argued [9] as experimentally established. They are also unaltered by the limit, as seen in (2). The main assumption is the addition of a new (heavy) chiral quark doublet , where the heavy isospin symmetry implies that , that is, equality of the Yukawa couplings. We ask whether large could be the source of EWSB, through the conceptual gap equation of Figure 1.
3.3.1. Ladder Approximation
In any case, we do not know the full propagator and vertex functions. We approximate the Goldstonefermion vertex as undressed, and the Goldstone propagator remains as , analogous to the QED treatment in previous section. This is in part aided by the insight that is a very tight bound state, which would be massless as long as the symmetry remains spontaneously broken. Similar to Figure 5, the gap equation for large Yukawa (vanishing ) coupling is depicted in Figure 6. Again, the external momentum flows through the loop.
The change from the symbolic or conceptual equation of Figure 1 is that, even with bare mass forbidden by gauge invariance (), there is a part for propagation, and we aim at solving for the quark propagator , given as which is of course of the same form as (11) for QED. The Goldstone boson is colorless, and, unlike the massless photon from electromagnetic gauge invariance for QED case, its masslessness is “bootstrapped” into the gap equation itself. Following similar steps as in Section 2, and assuming degeneracy, we obtain where placement of anticipates the Wick rotation, and stands as shorthand for , and likewise for . We have already used ; so, compared to massless QED, we now have to consider , or wave function renormalization effects; hence, we have to face a coupled set of equations for and . Note that we have kept a “Higgs” term for calculational purposes, applying Standard Model Higgs boson, , couplings. This is for purpose of later comparison with the work of Hung and Xiong [25], as well as for discussion of the dilaton case.
For our aim of bootstrap DSB, we simply drop the second term (no physical Higgs, or taking ), and so only Goldstone modes propagate in both equations. After angular integration and Wick rotation, one gets where Taking the limit in (30) and (31) to mimic the HungXiong approach of massless scalar doublet, We keep the notation of and in (33) and (34) to cover these two cases.
Analogous to Section 2, (32) can be put into differential form with the boundary conditions where prime stands for derivative.
At this point, we note that, if one ignores wave function renormalization, that is, (36), while forcefully setting in (35), then one has the same solution as in QED, with the change in critical coupling which is twice as high as for QED, and hence, superficially a “critical mass” GeV, which is above current LHC limits [14–20]. But it should be clear that the wave function renormalization term cannot be neglected.
3.3.2. Numerical Solution
Redefining , our coupled differential equations with B.C. become where dot represents derivative, and , .
Asymptotic Properties and Critical Coupling. Due to scale invariance, the differential equations are invariant under As a result, the solutions of the differential equations depend only on () and for given and . Thus, is a kind of integration constant. We will see that the most important feature of the solutions is that only special values (discontinuous values) of and are allowed for given boundary conditions.
If we take , the equations can be solved analytically, and the solution can be described as in the case of strong coupling QED with Landau gauge, (21)–(23). The property illustrated for should hold also for , where, depending on , should take on special discontinuous values to satisfy the gap equation for the cases of or .
To see this, we note that the term in the denominators is irrelevant. This is because for , the dependence of and is negligible due to the boundary conditions . Therefore, to understand the behavior of the solution, one can take and consider the differential equation with dropped as follows: where the equation for becomes independent from , but its solution affects .
The solution of is obtained analytically as follows: where is an integration constant which can be fixed by the B.C. for IR. Using the analytical solution, one can show that only discontinuous values of can satisfy the B.Cs. The “critical” value of can be easily obtained numerically, even without neglecting term in the denominators. Of course, since the solutions are found numerically, it is not a proof that one really has a “critical” value. The upshot is that only special values of the coupling can satisfy the coupled equations for given values of , for (or for ) and .
Our numerical solution gives corresponding to where the latter case is much higher. Here stands for “critical,” and our numerical values are extracted in the large and limit. Note that for the artificial case of (i.e., ), the critical value was , (40); hence, the effect of considering or wave function renormalization is quite nontrivial.
The values in (46) and (47) correspond to effectively taking , which is certainly not the range of validity for (46) as a descendent of Figure 1. That is, the conceptual foundation for Figure 1 is that, for momentum roughly up to somewhere below , corrections to the Goldstone boson propagator and vertex have been ignored. Nevertheless, at face value, if we naively apply the physical GeV, then (46) and (47) imply the mass values and 8.1 TeV, respectively, which are rather high. We drop the latter, “massless (or light) Higgs” case, not only because it is clearly out of reach for the LHC, but for theoretical reasons as we explain later. The lower bound nature of (48) would be explained subsequently.
3.4. Discussion
The large critical coupling of of (46) is somewhat surprising, resulting in the rather high critical mass of (48). We note that this is without the contribution of a light SM Higgs boson, which would put much higher. Before we touch phenomenology of such high chiral quark masses, and in so doing find an independent justification for such high critical Yukawa coupling, we offer some further discussion.
3.4.1. Comparison with Hung and Xiong
We can now make some comparison with, and offer a critique of, the approach of Hung and Xiong [25] (HX). We have mimicked the concept of HX by keeping a “Higgs” scalar contribution in (30) and (31), which resulted in the second case of (34) in the limit of , as compared with our case of interest, (33), where we drop the dependent term.
HX assumed the existence of a massless Higgs doublet, where our (35) and (36) with (34) should be a faithful representation. However, not only is the massless doublet assumed, HX also ignored wave function renormalization, that is, the term, in the treatment of their gap equation. Furthermore, the sign of our second integral in (30) disagrees with HX, suppressing the coefficient of in comparison. In the earlier work [9] that set up the gap equation of Figure 1, taking the numerics of HX, the estimate of (compare (40)) gave GeV, which is not too far above the current LHC bound. But with our sign for the second integral in (30), we would arrive at , or TeV, that is, a factor of higher. With our sign, the Higgs boson effect would cancel out part of the Goldstone effect, hence, requiring stronger Yukawa coupling.
But we have argued that it is not justified to ignore the wave function renormalization effect of . After all, the boson loop has momentum dependence, and so it would necessarily affect the factor. Thus, the previous simple numerics are incorrect. Keeping in our numerical study, hence, the coupled equations, a considerably higher critical is found. For the case of taking , (34), where we mimic HX’s massless Higgs doublet effect, the critical of (47) is almost 4 times as high as that for (46). In fact, we obtain the , which is quite different from 1.
Our criticism goes far deeper. Taking a scalar doublet as massless, such that superficially one has “scaleinvariance” as in strong QED, is totally ad hoc. Effectively one has to hold the parameters of the Higgs potential such that the Higgs field always remains massless. However, there is no principle by which this scaleinvariance or masslessness of the Higgs field can be maintained. After all, one is invoking large Yukawa couplings, which feed the notorious divergent quadratic corrections to the Higgs boson mass. The oneloop twopoint and fourpoint functions with quark in the loop would generate effective and selfcoupling terms for the Higgs field. With no explicit dynamical principle (such as gauge invariance for the case of QED), the assumption of a massless Higgs doublet as the agent of DSB is not only ad hoc, but clearly unsustainable.
In contrast, we see the merit, as well as the meaning, of our “bootstrap” gap equation. As long as we are in the broken phase, there is a massless Goldstone boson that couples with the Yukawa coupling . Treating as large, if a nontrivial solution to the gap equation is found (as we have illustrated earlier in the previous subsection), it in turn justifies the use of a massless Goldstone boson in the gap equation, which is why we affix the name “bootstrap.” In fact, the physical argument [9] was to view the Goldstone boson as an extremely tight ultrarelativistic bound state of heavy and from the broken phase, while enters the “bootstrap” gap equation to dynamically generate , hence, break the symmetry, and in the same stroke justify its own existence.
We also see that this argument for our bootstrap gap equation puts the existence of a light Higgs boson in doubt. That is, it seems rather difficult to keep it light, and one cannot ignore corrections to the Higgs propagator. At the foundation level [9], unlike the Goldstone boson, the experimental basis for the Higgs boson is rather recent. Even with the newly discovered [1, 2] 125 GeV boson, one has to distinguish between an SM Higgs boson versus a dilaton. Our numerical study also shows that keeping the Higgs term tends to raise the critical Yukawa coupling considerably, implying higher than the LHC collision energy. Thus, the light Higgs case of is rather problematic in bootstrap DSB. We will return to discuss the dilaton possibility later.
3.4.2. Physical Cutoff
The previous comparison with [25], and in particular the bootstrap nature of the Goldstone boson in the gap equation, illustrates that the limit would take us outside the range of validity of the gap equation itself. It is clear that, for timelike , there would no longer be a Goldstone boson. Thus, for the cutoff , one should not use the traditional language of . One probably should not contemplate “UVcompletion" at the current stage. The bootstrap gap equation is rather heuristically or physically argued. But it does not provide a theory of the heavy quark Yukawa coupling , employing it for DSB instead. Thus, we suggest a cutoff , where is some true New Physics scale where the origin of Yukawa couplings may be contemplated, but it is out of reach from the bootstrap DSB approach.
Viewed from a slightly different angle, this cutoff is related to the restoration of symmetry. The Goldstone boson couples to broken currents, but the factor of the Goldstone boson may vanish at some scale related to the scale where the Goldstone boson becomes unbounded, and symmetry is restored. Rather than a true that in principle extends to infinity, there exists a cutoff of the gap equation. We are in effect summing over the Goldstone boson correction to the selfenergy of the quark , when the Goldstone boson is still defined. As noted in [9], this picture does receive experimental support, in that no New Physics seem to be there below ~TeV scale. So, one sums up only the effect of the Goldstone boson, and nothing else.
The gap equation sums up the effect, from low to high momentum, of the correction by the Goldstone boson to the quark selfenergy. Equation (46) reflects taking this sum to . Since the summation is accumulative, if now one sums only to some , as we have argued, then the cumulative effect is less than summing to very large momentum above . We note that is a physical scale parameter that is external to the scaleinvariant gap equation. Nevertheless, we can plot the dependence of on the cutoff . From Figure 7, one can see that, for a lower cutoff, has to be higher than in (46). This is because, as the integration range is smaller, a larger value is needed to compensate. Thus, (46) gives a lower bound on . If we take , then , and which is higher than (48). We will return to discuss whether this could be an overestimate later.
3.4.3. Future Work
Up to now, we have been cavalier in the relation between and , treating it as . But is a physically measured quantity, and is yet to be experimentally measured. If electroweak symmetry is indeed dynamically broken by the large Yukawa coupling of a new heavy chiral quark , when is discovered in the future, likely . We then see that the actual v.e.v. value, , may not correspond to the critical value . This brings about the question of how scale invariance is actually broken in our gap equations, and whether there might be a dilaton [5–7, 45–49]. (When the 125 GeV hint emerged from 2011 LHC data, [45–47] already suggested that it might be a dilaton rather than the SM Higgs boson, while [48, 49] are from the (walking) technicolor perspective).
Rather than to approach this deeper problem, we try to obtain the decay constant of the Goldstone boson, which should be the same as the vacuum expectation value, . Following the PagelsStokar formula [50] naively, we obtain More generally, we write where , and we have scaled by (and redefined the function ), treating it as physical.
We can get back the “Yukawa” coupling (it should really be denoted as , and the question is whether ) for the input to the gap equation, or If the system is really scaleinvariant, the r.h.s. of (52) is a function of and . In order to satisfy the gap equation, is obtained as a function of . Namely, it should not depend on explicitly. Taking the cutoff , the equation becomes iterative for . Therefore, solving the gap equation, we obtain a prediction for the heavy quark mass. But technical issues remain. Is a physical mass? What about the infrared cutoff? Can our assumption of be maintained selfconsistently? Our work is far from complete, and we leave these theoretical questions to the future.
4. New Phenomena:
The stringent limit of GeV/c^{2} [14–20] is already above the perturbative, treelevel partial wave unitarity bound (UB) that is nominally around 550 GeV/c^{2} [21]. With TeV scale heavy quark masses, the actual UB violation (UBV) in the high energy limit for scattering may be out of reach. Instead, the question to ask is should the current search strategy for ultraheavy quark at the LHC be modified? Of course, with the advent of the 125 GeV boson at the LHC, the search for the four generation quarks has been blunted, and the search effort is being reshuffled to search for vectorlike quarks, where flavor changing neutral current (FCNC) decays to and Higgs bosons need to be studied. We maintain, however, that SM has builtin absence of FCNC, both for the (only chiral fermions) and Higgs (single Higgs doublet). There is some merit to stick to this, while our bootstrap equation has even disposed of the Higgs doublet altogether.
So, what if there are heavy chiral quarks in Nature at the 23 TeV level? Can they be discovered at the LHC? We draw on the analogy with the proton to argue [52] that ( is the longitudinal component of vector boson) may be the new signature at the LHC.
The coupling [53, 54] gives , which is very large and quite close to the “Yukawa coupling,” , which is slightly larger than . Although ( GeV is the electroweak symmetry breaking scale) from the current bound is not yet as large, drawing analogy with annihilation, we expect that may be the dominant process for GeV. It is also realizing the fact that is of similar strength to , that such strong couplings already exist in Nature, which gives some confidence to our very large critical Yukawa coupling strength.
4.1. Phenomenology of
The phenomenon for annihilation is unfamiliar to the average particle physicist. One tends to think of annihilation into photons (much suppressed by of QED) or gluons. But even for the latter, it is not practical with total energy of ~1.88 GeV and in consideration of detection of final states. Certainly, would annihilate into mesonic resonances. However, all mesonic resonances basically end up as pions. Thus, one can safely conclude that in general.
Indeed, it is observed that annihilation [51, 55] goes mainly into pions. However, the features are rather surprising, even for the nuclear and hadron physicists that worked on the subject from the 1950s to the 1990. It is found that goes via a “fireball.” The salient features of the annihilation “fireball” are (see Figure 8)(i)size of order ; (ii)temperature MeV; (iii)average number of emitted pions ; (iv)a softpion factor modulates the MaxwellBoltzman distribution for the pions.
It is worthwhile to elucidate these features a little further. The size means that, when the and meet to annihilate, destined to shed the and content, the region of annihilation extends over a region ~1/m_{π}. The system seems to thermalize to a temperature of order 120 MeV, hence, “loses memory” of its origins, and the emitted pions carry momenta that satisfy a thermal distribution. This rapid thermalization probably takes place due to the rather large (as well as ) coupling, while the suppression [56] (satisfied rather well by data; see Figure 12 of [51]) for low pion momentum from the thermal distribution reflects nothing but the Goldstone nature of pion couplings. That is, the as Goldstone boson couples derivatively, hence, cannot get emitted at zero momentum. This seems to explain the enhancement factor of 1.3 for the mean kinetic energy beyond equipartition expectation of . Thus, the relatively high MeV gives rise to , as compared to the maximal allowed number of pions, .
At a more refined level, it is found that and , with ; that is, more neutral pions are emitted than charged ones. Remarkably, the pion multiplicity distribution appears Gaussian, with . More specifically [57], is argued from statistical models [58]. Thus, gives a good fit to data [51], which is given in the first row of Table 1. Note the minute 2body fraction, while the pion multiplicity cuts off above 8.

This successful “statistical model” which accounts for gross features of annihilation goes back to Fermi [59], who considered a system of noninteracting pions. It has been refined through the years, and the strong interactions of the pions do play a major role. One final aspect is a focusing of incoming waves by attractive potential that leads to strong absorption in a smaller region than originally suggested.
4.2. Analog
We mean by a lefthanded chiral doublet (with corresponding righthanded weak singlets) that is degenerate in mass, thereby possessing a heavy isospin symmetry , much like the nucleon . To draw true analogy with the case, the Yukawa coupling should be of order 1314; that is, TeV, in accordance with findings of the bootstrap gap equation. However, for sake of phenomenology, we will assume that analogous phenomenon already appears for 1 TeV; hence, we consider TeV.
With Higgs mechanism already established, the Goldstone boson carries with it an effective length scale (assuming symmetry, we take and ignore weak gauge couplings , compared with ), which should define the size of the annihilation fireball. Compared with , here where is the weak gauge coupling. Thus, the size of the fireball is controlled by random parameters such as or that are unrelated to the underlying annihilation dynamics.
The fireball temperature is harder to assess. Noting that , likely , where is the electroweak transition temperature. By this analogy, however, one notes that arises from the detailed underlying theory for hadron phenomena (which includes ), QCD. Even if EWSB arises from strong Yukawa coupling [8, 9], , we do not yet have an underlying theory for itself. Thus, we do not have a good handle on , except that it is in the 100 GeV scale, of order .
The Goldstone factor should still modulate the thermal distribution. But because of the smallness of compared with , the modulation is considerably milder than the case, and so should be closer to . We shall therefore take as nominal which can be interpreted as either (here 1.3 corresponds to ) or . The latter would give 170 GeV, which is not so different from (55). We stress, however, that the fireball temperature could be 1.5, even twice as high, and should be determined eventually by experiment.
Assuming (55) but without applying the 1.3 enhancement factor over equipartition (as was done for the case of ), we take GeV; hence, GeV, or with . For TeV, or TeV, and this corresponds to where we artificially keep three digits of significance for generating a “realistic” multiplicity distribution. Assuming (53) and (54), we have , and the multiplicity distribution is for TeV. We note that a higher fireball temperature would result in lower average multiplicity and a narrower distribution (controlled by ).
We illustrate the process in Figure 8 (gluon emission discussed later) and tabulate the multiplicity distributions in Table 1. For TeV (second row of Table 1 marked by ), about 90% of annihilations go into 5–8 prongs of . Several s should be considerably above 300 GeV momentum, while 4prong events (at 6%) are in general composed of s with momentum ~500 GeV. Therefore, tagged “fat” jets, , should become a useful tool for identifying these multi events. For TeV (third row of Table 1 marked by ), again over 90% of annihilations go into 10–15 prong s, which is a rather large number. For 9–12 prong events (at ~50%), a significant number of s would have momentum above 400 GeV, while for higher multiplicity, many should still carry momentum higher than the mean, (56). These high multiplicity events would be possible hallmark for heavy production.
4.3. LHC Prospects
At the moment, conventional wisdom has turned against searching for fourth generation quarks per se, because of the SMlike Higgs signal, even though a dilaton interpretation is still possible. Our discussion, however, point towards a possible new type of signature.
If our analogy with annihilation is already realized for TeV, then even at 8 TeV running of LHC, where of order data is expected in 2012 for both ATLAS and CMS, one could already get a hint. The crosssection is of order a couple fb; so, one might observe some number of 4 or more tagged jet () events, with additional jet multiplicity that are less well tagged. The competing modes would be regular production, followed by “free quark decay,” for example, (assuming ) , or [60]; we shall assume CKM hierarchy for simplicity; hence, , and , transitions are ignored. We see that the jet multiplicity is lower, associated with isolated high jets, and practically no jets or . In contrast, does not have isolated jets (jets would come in pairs at lower fraction, to form a from ), and jet multiplicity is higher and tends to have jets (the analogy with suggests a slight excess of over (half the) ; however, the mass is heavier than the , and so this point is to be determined by experiment). We expect that the fireball process would dominate over the free quark decay process, as we would argue shortly.
We have demonstrated in Section 3 that if the heavy chiral quarks themselves are responsible [9] for dynamical EWSB, then TeV is required [8]. Our earlier analogy with the “Yukawa” coupling suggests TeV. If so, the prospects for the 2012 LHC run at 8 TeV are not good, and one would have to wait for the 1314 TeV run, expected by late 2014. Running the HATHOR code [61] for production, we estimate the 14 TeV cross sections to be of order 50–60 fb for TeV, dropping to ~3 fb for TeV, and 0.20.3 fb for TeV. From to 4 TeV, one quickly runs out of parton luminosity. Note that production dominates over production, as the valence quark supplies the needed large parton momentum fraction.
From the cross section and expected LHC luminosities, for TeV, again we do not foresee a problem for discovery. Note that assuming symmetry, that is, near degeneracy of and , then (i) decay:suppressed by both phase space and small Goldstone momentum; (ii):suppressed by CKM element (), and with no sign of New Physics in , , and , one expects [62, 63] such CKM elements to be less than 0.1.
In contrast, once pulls the heavy quark pair out of the vacuum, the pair “sees" a cross section of order , which is at the level. With production, there is Yukawa attraction [24] between that mimics the focusing attraction for . Thus, there is good likelihood that , that is, , would dominate over free quark decay.
We comment that the produced is likely in a coloroctet state; hence, it would need to shed color. However, gluons have no way to sense the GeV (or higher) of the fireball, which is of electroweak nature. Instead, the heaviness of means gluon radiation is suppressed (heavy quark symmetry). We illustrate gluon radiation in Figure 8 but expect the associated gluonjet to be soft and does not provide a discriminant.
In case TeV, one quickly runs out of parton luminosities (higher energy would be preferred!); hence, one would need high luminosity running of LHC at 14 TeV. However, the situation needs not be so pessimistic; the very large Yukawa coupling suggests the existence of bound states below . For example, as discussed in [24], there is likely an isos