Abstract
We examine the dynamics of quarks and gauge fields in the lowest energy states in the QED and QCD interactions by combining Schwinger’s longitudinal confinement in (1+1)D with Polyakov’s transverse confinement in (2+1)D in a “stretch (2+1)D” flux tube model in (3+1)D. For such QED and QCD systems in the flux tube configuration with cylindrical symmetry, we separate out the transverse and longitudinal degrees of freedom, approximate the non-Abelian QCD in the quasi-Abelian approximation, and solve the derived equations to study the collective excitations. We find stable collective QED and QCD excitations showing up as confined QED and QCD mesons, in support of previous theoretical studies and recent observations of the anomalous hypothetical X17 and E38 particles. Future theoretical lattice gauge calculations of QED in (3+1)D with the inclusion of the Schwinger longitudinal confinement mechanism and experimental confirmation of the hypothetical X17 and E38 particles will shed definitive light on quark confinement in the QED interaction in (3+1)D.
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This manuscript has no associated data or the data will not be deposited. [Authors’ comment: All data generated during this study are contained in this published article.]
Notes
Because quarks and antiquarks cannot be isolated, the production of a \(q{\bar{q}}\) pair can occur only at certain CM eigenstate energies, \(\sqrt{s }(q{\bar{q}})\), of confined and bound \(q{\bar{q}}\) systems, such as in a QED meson or a QCD meson. At other energies different from confined and bound eigenstate energies, the q and \({\bar{q}}\) do not exist. Hence, a quark and an antiquark cannot be produced at energies that are not eigenenergies of bound QCD or QED mesons.
We adopt here the notations that unless stated otherwise, \(g^\lambda \) is actually \(g_{{}_{\textrm{2D}}}^\lambda \), the coupling constant in 1+1 dimensions, and \(g_{{}_{\textrm{4D}}}^\lambda \) is the coupling constants in 3+1 dimensions. The superscript \(\lambda \) specifies the interaction, with \(\lambda =0\) for QED and \(\lambda =1\) for QCD. The strong coupling constant is \(\alpha _{{}^{\textrm{QCD}}}=(g^{{}_{\textrm{QCD}}}_{{}_{\textrm{4D}}})^2/4\pi \) and the fine structure constant is \(\alpha _c=\alpha _{{}^{\textrm{QED}}}=(g_{{}_{\textrm{4D}}}^{{}_{\textrm{QED}}})^2/4\pi =(-e_{{}_{\textrm{4D}}}^{{}_{\textrm{QED}}})^2/(\hbar c)=1/137\). As pointed out in [38, 41, 172, 173] and Eq. (67), \(g_{{}_{\textrm{2D}}}^\lambda \) and \(g_{{}_{\textrm{4D}}}^\lambda \) are approximately related by the flux tube radius \(R_T\) as \((g_{{}_{\textrm{2D}}}^\lambda )^2=(g_{{}_{\textrm{4D}}}^\lambda )^2/(\pi R_T^2)\), when the confining flux tube of radius \(R_T\) is idealized as an open string without a structure.
There is a factor 2 on the left-hand side of the trace relation, \(2\textrm{tr} \{t^a t^b\} \,= \,\delta ^{ab}\), for the generator \(t^a\) and \(t^b\). For the convenience of notation, we shall define the operation “Tr trace” over the color space as \(Tr_\textrm{color} (t^a t^b)\) \( \equiv \)2tr\( \{t^a t^b\} \,= \,\delta ^{ab}\), when we calculate the trace of the product of generators \(t^a t^b\) in the color space.
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Acknowledgements
The authors would like to thank Prof. Y. Jack Ng for helpful communications. CYW’s research was supported in part by the Division of Nuclear Physics, U.S. Department of Energy under Contract DE-AC05-00OR22725 with UT-Battelle, LLC.
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Cheuk-Yin Wong’s research has been supported in part by UT-Battelle, LLC, under contract DE-AC05-00OR22725 with the US Department of Energy (DOE). The US government retains and the publisher, by accepting the article for publication, acknowledges that the US government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan (http://energy.gov/downloads/doe-public-access-plan), Oak Ridge, Tennessee 37831, USA.
Appendices
Appendices
Appendix A: Separation of quark transverse and longitudinal equations of motion in (3+1)D
To separate out transverse and the longitudinal degrees of freedom, we follow methods used previously by Wang, Pavel, Brink, Wong, and many others [150,151,152,153,154]. We employ the Weyl representation of the gamma matrices in Eq. (11) and write the quark field in terms of the transverse functions \(G_{\{1,2\}}({\varvec{r}}_\perp )\) and the longitudinal functions \(f_\pm (X )\) as
where \(\varvec{r}_\perp = \{x^1,x^2\}\), \(X = \{x^3,x^0\}\). Using the Weyl representation of the gamma matrices as given in Eq. (10), we obtain
The quark Lagrangian density becomes
where \(\varPi ^\mu =p^\mu + g A^\mu (x)\). The minimization of the action integral by variations with respect to \(f_\pm ^*\) and \(G_{\{1,2\}}^*\) leads to
We sum over \(G_1^*(\varvec{r}_\perp )\) \(\times \) (A.3) + \(G_2^*(\varvec{r}_\perp )\) \(\times \) (A.4) and perform an integration over the transverse coordinates. Similarly, we sum over \(G_1^*(\varvec{r}_\perp )\) \(\times \) (A.5) + \(G_2^*(\varvec{r}_\perp )\) \(\times \) (A.6) and perform an integration over the transverse coordinates. We get
From the second terms in each of the above two equation, we note that we can separate out the longitudinal and transverse equations by introducing the separation constant \(m_T\) defined by
Because of the normalization condition Eq. (12) for \(G_{\{1,2\}}\), the above equation can be rewritten as
The above is zero if the two terms in the integrand are zero, and we obtain the eigenvalue equations for the transverse functions \(G_{\{1,2\}}(\varvec{r}_\perp )\),
We apply \( (\varPi ^1+i\varPi ^2)\) on the first equation and \( (p^1+ip^2)\) on the second equation and we get
We have then
where \(\varPi _T^2=(\varPi ^1)^2+(\varPi ^2)^2\) is the square of the transverse momentum. Upon the introduction of the constant of separation \(m_T\), Eqs. (A.7a) and (A.7b) become
In the above two equations, the operators \(\varPi ^\mu \) with \(\mu =0,3\) are actually \(\varPi _{{}_{\textrm{4D}}}^\mu \)=\(p^\mu + g_{{}_{\textrm{4D}}} A_{{}_{\textrm{4D}}}^\mu (\varvec{r}_\perp ,X)\) where the gauge field \(A_{{}_{\textrm{4D}}}^\mu \) is a function of the (3+1)D coordinates \((\varvec{r}_\perp ,X) \) and \(g_{{}_{\textrm{4D}}}\) is the dimensionless coupling constant in (3+1)D space-time. Upon carrying out the integration over the transverse coordinates \(\varvec{r}_\perp \), the above two equations can be cast into the Dirac equation for a particle with a mass \(m_T\) in (1+1)D space time of X coordinates by identifying the terms integrated over the transverse coordinates as the corresponding gauge fields \(A_{{}_{\textrm{2D}}}^\mu \) in the (1+1)D space-time with the coupling constant \(g_{{}_{\textrm{2D}}}\)
where \(A_{{}_{\textrm{2D}}}(X)\) is the solution of the Maxwell equation for the gauge fields in (1+1)D space-time. By comparing the Maxwell equations in (3+1)D and (1+1)D space time in Appendix B, it can be shown in Appendix B that the coupling constant \(g_{{}_{\textrm{2D}}}\) is then determined by
We note that the coupling constant \(g_{{}_{\textrm{2D}}}\) acquires the dimension of a mass. By such an introduction of \(A_{{}_{\textrm{2D}}}^\mu \) and \(g_{{}_{\textrm{2D}}}\), Eqs. (A13a) and (A13b) become
where \(\varPi _{{}_{\textrm{2D}}}^\mu =p^\mu +g_{{}_{\textrm{2D}}} A_{{}_{\textrm{2D}}}^\mu (X)\), with \(\mu =0,3\). Equations (A.10), and (A.14) (which correspond to Eqs. (17) and (22) in Section III) are the set of transverse and longitudinal equations of motion for the quark field \(\varPsi \) in (3+1)D space for our problem.
Appendix B: Relation between quantities in (1+1)D and (3+1)D
We shall examine the relation between various quantities in (1+1)D and (3+1)D. The time-like component of the quark current is the quark density, and the density in (3+1)D involves the transverse spatial distribution while the density in (1+1)D does not involve the transverse spatial distribution.
We consider the quasi-Abelian approximation of the non-Abelian QCD gauge field in so that the QED and QCD gauge fields can be represented in terms of only the commuting \(\tau ^0\) and \(\tau ^1\) components, as discussed in Sect. 8.2. To make the problem simple, we consider lowest-energy state systems with cylindrical symmetry so that we can write our wave function of the quark fields in the form of Eq. (11), and the transverse currents \(j^1\) and \(j^2\) are given in terms of the basic functions \(G_{\{1,2\}}\) and \(f_\pm \) by
For our problem, we choose to examine the quark-QED system in which the quarks and antiquarks reside in the zero mode with \(m_T=m\), and with the quark wave functions given by (66). For these zero mode states, \(G_{\{1,2\}}\) are spinors aligned in the longitudinal direction. As a consequence, when \(G_1(\varvec{r}_\perp )\) is non-zero, \(G_2(\varvec{r}_\perp )\) is zero, and vice-versa. The product \(G_1^* G_2\) and \(G_2^*G_1\) are always zero for quark and antiquark in the lowest energy zero mode states. Therefore for these lowest energy states the currents in the direction of \(x^1\) and \(x^2\) are zero. We assume that the transverse gauge fields \(A^{\{1,2\}}\) are determined by the transverse dynamics of their own to yield the solutions of the transverse stationary states \(G_{\{1,2\}}(\varvec{r}_\perp )\). Within the cylindrical flux tube, the gauge fields are only a weak function of the transverse coordinates so that it is necessary to consider the Maxwell equation only for \(\nu , \mu \)=0,3 in (3+1)D with
With the quark field \(\varPsi _{{}_{\textrm{4D}}}\) as given by Eq. (11), the quark currents in (3+1)D are given by
From the 2D action \({{{\mathcal {A}}}_{{}_{\textrm{2D}}}}\) in Eq. (43), we can derive the Maxwell equation in (1+1)D as given by
for \(\nu ,\mu =0,1\) in (1+1)D. With the quark field \(\psi _{{}_{\textrm{2D}}}\) as given by Eq. (26), the quark currents \(j_{{}_{\textrm{2D}}} ^\nu (X)\) in (1+1)D are given by
Comparison of the quark currents in (3+1)D and (1+1)D in Eqs. (B.3), (B.4) (B.6), and (B.7) gives
Then, substituting the above equation into Eq. (B.2), we obtain for \(\nu ,\mu =0,3\) in (3+1)D
The above equation in (3+1)D would be consistent with the (1+1)D Maxwell equation (B.5) if for \(\mu =0,3\),
On the other hand, the equation of motion in Eqs. (A14) would require that \(g_{{}_{\textrm{4D}}}\) and \(g_{{}_{\textrm{2D}}}\) are related by
The consistency of both equations (B.10) and (B.11) requires \(g_{{}_{\textrm{4D}}}\) and \(g_{{}_{\textrm{2D}}}\) to satisfy the relation
which is Eq. (21).
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Wong, CY., Koshelkin, A.V. Dynamics of quarks and gauge fields in the lowest-energy states in QED and QCD interactions. Eur. Phys. J. A 59, 285 (2023). https://doi.org/10.1140/epja/s10050-023-01180-8
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DOI: https://doi.org/10.1140/epja/s10050-023-01180-8