Hamiltonian approach to QCD in Coulomb gauge at zero and finite temperature

I report on recent results obtained within the Hamiltonian approach to QCD in Coulomb gauge. By relating the Gribov confinement scenario to the center vortex picture of confinement it is shown that the Coulomb string tension is tied to the spatial string tension. For the quark sector a vacuum wave functional is used which results in variational equations which are free of ultraviolet divergences. The variational approach is extended to finite temperatures by compactifying a spatial dimension. For the chiral and deconfinement phase transition pseudo-critical temperatures of 170 MeV and 198 MeV, respectively, are obtained.


Introduction
Understanding the QCD vacuum is still one of the big challenges of theoretical physics. Although substantial progress has been made during the last two decades we are far from rigorously understanding the essential features of the QCD vacuum: confinement and spontaneous breaking of chiral symmetry. Under normal conditions quarks and gluons are confined inside hadrons, and the hadrons receive most of their mass through the mechanism of spontaneous breaking of chiral symmetry. When baryonic matter is heated up or strongly compressed, hadrons melt and a plasma of quarks and gluons is formed. This deconfinement phase transition is accompanied by the restoration of chiral symmetry. We have learned a lot about this phase transition from lattice calculations at finite temperatures and vanishing baryon density, i.e. along the temperature axis of the phase diagram, see Fig. 1. However, the lattice approach fails at finite chemical potential due to the so-called sign problem (the quark determinant becomes complex). To understand the deconfinement phase transition at finite chemical potential continuum approaches are thus required, which do not face the sign problem and are able to deal with a non-zero chemical potential. I will present here such a continuum formulation, namely the Hamiltonian approach. In fact, this method is currently being developed and tested at finite temperatures where it can be compared to available lattice calculations, and I will not yet present results for finite chemical potential. In the first part of my talk I will study the QCD vacuum within this approach and will then extend it to finite temperatures.
One may ask for the benefit of the Hamiltonian approach as compared to the more common functional integral approach, which is so elegant for perturbation theory and which is also the basis for the lattice calculations. From quantum mechanics we know that solving the Schrödinger equation is usually much simpler and much more efficient than calculating the functional integral directly. For example, it is quite easy to solve the Schrödinger equation for the hydrogen atom, while calculating the corresponding functional integral directly is exceedingly complicated. Also in non-perturbative continuum quantum field theory the Hamiltonian approach is in my opinion more efficient. In my talk I will use the Hamiltonian approach to QCD in Coulomb gauge first to study the QCD vacuum by means of a variational solution of the Yang-Mills Schrödinger equation. Then I will extend this approach to finite temperatures by compactifying a spatial dimension. I will first illustrate the method by means of free bosons and fermions and then apply it to QCD at finite temperatures, where I will mainly concentrate on the calculation of the effective potential of the Polyakov loop.

Hamiltonian approach to QCD in Coulomb gauge
The Hamiltonian approach to quantum field theory is based on the canonical quantization. We illustrate this formalism first for the Yang-Mills theory, which is defined by the classical action S = 1 4 − d 4 x F a μν F aμν . Here, F a μν = ∂ μ A a ν − ∂ ν A a μ + g f abc A b μ A c ν denotes the non-Abelian field strength. For the canonical quantization, the gauge fields are considered as the "coordinates". The canonical conjugate momenta are introduced in the standard fashion by Π a μ (x) = δS /δȦ aμ (x). For the spatial components of the gauge field A a i (x) these momenta coincide with the color electric field Π a i (x) = −E a i (x), while the momentum corresponding to the temporal component of the gauge field A a 0 (x) vanishes. The latter causes problems in the canonical quantization which, however, can be circumvented by imposing Weyl gauge A a 0 (x) = 0. One finds then the following classical Hamiltonian of Yang-Mills theory where B a i = 1 2 ε i jk F a jk is the color magnetic field. The theory is quantized by imposing the usual canonical commutation relations, i.e.
In the coordinate representation the momentum operator is therefore realized by Π a k (x) = δ/(iδA a k (x)). Because of the Weyl gauge A a 0 (x) = 0, Gauß's law is lost as an equation of motion and has to be imposed as a constraint on the wave functional HereD ab is the covariant derivative in the adjoint representation of the gauge group, and the operator on the left hand side,D · Π, is nothing but the generator of time-independent (space-dependent) gauge transformations. Furthermore, ρ m is the color charge density of the matter field. In the absence of a matter field the right hand side of eq. (4) vanishes and the wave functional has to be invariant under time-independent gauge transformations ψ[A U ] = ψ[A]. With the canonical momentum replaced by the operator Π a k (x) = δ/(iδA a k (x)), eq. (1) becomes the Hamilton operator of Yang-Mills theory. With this operator one has to solve then the Schrödinger equation in the Hilbert space of gauge invariant wave functionals, which has the usual scalar product known from quantum mechanics where D A denotes the functional integral over (time-independent) spatial components of the gauge field. One is mainly interested in the solution of the Schrödinger equation (5) for the ground state (vacuum). There have been attempts to solve the Schrödinger equation directly for the vacuum in the Hilbert space of gauge invariant wave functionals. However, so far these attempts have been successful only in 2+1 dimensions [1]. In 3+1 dimensions it seems extremly difficult to find gauge invariant representations of the wave functional except for some limited cases [2]. Therefore it is much more efficient to fix the gauge, and a convenient choice for this purpose is the Coulomb gauge ∂ · A = 0. This condition can be implemented in the scalar product (6) by the standard Faddeev-Popov method resulting in Here the integration is now over the transversal components of the gauge field A ⊥ only and is the Faddeev-Popov determinant in Coulomb gauge. The Coulomb gauge fixing basically corresponds to a transition from Cartesian coordinates to curvilinear coordinates and the Faddeev-Popov determinant represents the Jacobian of this transformation. Even if the longitudinal components of the gauge field are eliminated in Coulomb gauge the momentum operator still contains also a longitudinal component Π . From Gauß's law one finds for the longitudinal momentum operator when it acts on a wave functional With this relation (9) one finds for the Yang-Mills Hamiltonian in Coulomb gauge [3] where arises from the kinetic energy of the longitudinal components of the momentum operator and is usually referred to as the Coulomb term. Here ρ(x) is the total color charge density, which includes besides the matter charge density ρ m (x) also the charge density of the gauge field ρ a , which exists obviously only in non-Abelian gauge theories. In the case of QED where the Faddeev-Popov operator becomes the Laplacian (−Δ), the term eq. (11) produces precisely the Coulomb potential between electric charge densities ρ.
The Coulomb gauge fixed Hamiltonian (10) is obviously more complicated than the original gauge invariant one (1). First, the Faddeev-Popov determinant appears in the kinetic energy of the transversal degrees of freedom [the first term in eq. (10)] and, second, the kinetic energy of the longitudinal degrees of freedom (11) is a highly non-local object. Furthermore, the Faddeev-Popov determinant appears also in the scalar product (7). This is the price one has to pay for the gauge fixing. Nevertheless it is still more convenient to work with this more complicated gauge fixed Hamiltonian than with gauge invariant wave functionals. Let us stress that by implementing Gauß's law in the gauge fixed Hamiltonian, all consequences of gauge invariance are fully taken into account.

Variational solution of the Yang-Mills Schrödinger equation for the vacuum
Variational calculations within the Hamiltonian approach to Yang-Mills theory in Coulomb gauge were initiated by D. Schütte in Ref. [4] who used a Gaussian trial ansatz for the vacuum wave functional. By minimizing the energy density he derived a closed set of coupled integral equations for the gluon propagator, the ghost propagator and the Coulomb potential. Later on, Ref. [5] followed the approach of Ref. [4] by using the same ansatz for the vacuum wave functional, but in addition provided the first numerical solution of the resulting integral equations. In Refs. [6,7] we have developed in our group a variational approach to Yang-Mills theory in Coulomb gauge, which differs from previous approaches: i) in the ansatz for the vacuum wave functional, ii) in the treatment of the Faddeev-Popov determinant 1 and iii) in the renormalization. Our trial ansatz for the vacuum wave functional is given by where ω(x, y) is a variational kernel, which is determined by minimizing the energy density. The ansatz (12) has the advantage that the static gluon propagator is given by the inverse of the kernel ω A a k (x)A b l (y) = δ ab t kl (x) where t kl (x) = δ kl − ∂ x k ∂ x l /∂ 2 x is the transversal projector. From the form of the static gluon propagator (13) it follows that the Fourier transform of ω(x, y) represents the single-particle gluon energy. Minimizing the energy density with respect to ω(x, y) yields the result shown in Fig. 2 (a) [8]. For large momenta the gluon energy behaves like the photon energy ω(p) ∼ |p| while at small momenta it diverges ω(p) ∼ 1/|p| implying the absence of free gluons in the infrared, which is a manifestation of confinement. The numerical calculation carried out in Ref. [9] shows that the Coulomb term (11) can be ignored in the Yang-Mills sector. Then the gluon gap equation resulting from the minimization of the energy density is given by where χ(p) is the ghost loop, which is diagrammatically represented in Fig. 3. The gap equation (14) has the form of the dispersion relation of a relativistic particle except that the (effective) mass of the particle is replaced by the ghost loop χ(p). The ghost propagator is given here as the vacuum expectation value of the inverse Faddeev-Popov operator and is represented by where d(−Δ) is the so-called ghost form factor. Obviously, this form factor contains all the deviations from QED where the Faddeev-Popov operator is just given by the Laplacian. For large momenta the ghost form factor approaches unity while it diverges like 1/p in the infrared and thus fulfills the so-called horizon condition d −1 (p = 0) = 0 [10]. Contrary to other gauges, in Coulomb gauge the ghost form factor d has a physical meaning: Its inverse represents the dielectric function of the Yang-Mills vacuum, Ref. [11]. The horizon condition guarantees that the dielectric function vanishes in the infrared ε(p = 0) = 0, which implies that the Yang-Mills vacuum is a perfect color dielectricum or a so-called dual superconductor. In this way the Hamiltonian approach in Coulomb gauge relates to the dual superconductor picture of confinement introduced many years ago by Mandelstam [12] and 't Hooft [13]. The form of the dielectric function obtained here is in accord with the phenomenological bag model picture of hadrons [14]: On the one hand, inside the hadrons i.e. at small distances, the dielectric function equals unity which is the value of a normal vacuum, as in QED and also in QCD without matter, due to asymptotic freedom. On the other hand, outside the physical hadrons the infrared value ε(p = 0) = 0 corresponding to a confining vacuum is realized. Indeed for a medium with ε = 0 the electrical displacement D = εE vanishes implying by Gauß's law, ∂ · D = ρ f ree , that no free color charges can exist. Figure 4 compares the results of the variational calculation with the lattice results for the gluon propagator. The lattice results [15] can be nicely fitted by Gribovs' formula [16] with a mass scale of M 880 MeV. The gluon energy (dashed line) obtained with the Gaussian trial wave functional agrees quite well with the lattice data in the infrared and in the ultraviolett regime but misses some strength in the mid-momentum regime. This missing strength is largely recovered when a non-Gaussian wave functional is used, Ref. [17], which includes in the exponent of the trial wave functional also cubic and quartic terms in the gauge potential. When non-Gaussian wave functionals are used, Wick's theorem is no longer valid. In Ref. [17] this problem was circumvented by exploiting generalized Dyson-Schwinger equations to express the various n-point functions occuring in the expectation values of operators like the Hamiltonian in terms of the variational kernels occuring in the exponent of the wave functional. One finds then the full curve in Fig. 4, which fits the lattice data in the mid-momentum regime much better than the Gaussian ansatz.   The part of the Coulomb Hamiltonian (11), which is quadratic in the charge density of the matter field ρ m represents a two-body interaction which is induced by the Yang-Mills vacuum. The Faddeev-Popov determinant drops out from this part of the Coulomb term and its vacuum expectation value yields the static color charge potential  Figure 2 (b) shows the resulting quark-antiquark potential obtained from our variational Yang-Mills vacuum solution [8] when the vacuum expectation value is factorized resulting in where G(x, y) is the ghost propagator (15). The obtained potential rises linearly at large distances with a coefficient given by the so-called Coulomb string tension σ C , which on the lattice is measured to be a factor of 2 . . . 3 larger than the Wilson string tension σ ≈ (440 MeV) 2 [18]. At small distances the potential behaves like the Coulomb potential as expected from asymptotic freedom. So far, we have seen signals for confinement both in the gluon propagator and in the static Coulomb potential. However, to really show that our approach yields confinement we have to calculate the vacuum expectation value of the Wilson loop which is the order parameter of confinement: In the confining theory this quantity decays exponentially with the area A enclosed by the loop C with a coefficient referred to as Wilson string tension σ. An area law implies a linear rising potential with a slope given by σ. On the other hand in the deconfined phase the expectation value decays only with the perimeter P of the loop. Unfortunately the Wilson loop is difficult to calculate in a continuum theory due to path ordering. In Ref. [19] an approximate evaluation of the Wilson loop was carried out and the potential extracted from the Wilson loop is shown in Fig. 5 (a). This method works only up to intermediate distances where the small distance Coulomb behavior of the potential has not yet died out. When the perturbative part is removed, however, one does indeed observe the linear rising potential shown in Fig. 5 (b). An order parameter (or more precisely disorder parameter) of confinement, which can be easier calculated in the continuum is the 't Hooft loop [20]. The operatorV(C) corresponding to the 't Hooft loop is defined by the relationV for any two closed loops C 1 and C 2 . Here W(C 2 ) is the Wilson loop (19) and z is a non-trivial center element of the gauge group. Furthermore, L(C 1 , C 2 ) is the Gaussian linking number, which is nonzero when the two loops in the argument are non-trivially linked. The 't Hooft loop operatorV(C) is dual to the Wilson loop in the sense that a perimeter law implies confinement while an area law implies deconfinement. 't Hooft gave an explicit realization of the loop operatorV(C) on the lattice. In Ref. [21] a continuum representation ofV(C) was derived, where Π = δ/(iδA) is the momentum operator of the gauge field and A(C) is the gauge potential of a so-called thin center vortex, which is a closed magnetic flux line located at the loop C. The center vortex field A(C) is defined by its Wilson loop . In Ref. [22] the 't Hooft loop was calculated with the wave functional obtained from our variational approach and indeed a perimeter law was found.

Variational approach to QCD in Coulomb gauge
The approach presented above for the Yang-Mills sector can be extended to full QCD. The Hamiltonian of QCD in Coulomb gauge is given by Here H Y M is the Hamiltonian of the transversal gluon degrees of freedom given in eq. (10). Furthermore, H C is the Coulomb term (11) where, however, now the charge density of the matter field is given by that of the quarks ρ a m (x) = ψ † (x)t a ψ(x) .
Here, ψ(x) is the quark field and t a denotes the generators of the gauge group in the fundamental representation. Finally,

ICNFP 2015
is the Dirac Hamiltonian of the quarks interacting with the spatial gauge field A. In the following let us concentrate on the quark sector. For the quark vacuum wave functional we have used recently the following variational ansatz [23] Here ψ ± denote the positive and negative energy components of the quark Dirac spinor, while s, v, w are variational kernels to be determined by minimizing the QCD energy density. For v = w = 0 the ansatz reduces to a BCS type of wave functional, which was used in Refs. [24], [25], [26]. Furthermore, for w = 0 the ansatz was used in Refs. [27], [28]. There it was found that the inclusion of the coupling of the quarks to the transversal gluons in the vacuum wave functional substantially increases the amount of chiral symmetry breaking. With the quark wave functional (28) we have calculated the expectation value of H QCD up to two loops and carried out the variation with respect to the kernel s, v, w. This results in three coupled equations, where the equations for v and w can be explicitly solved in terms of the scalar kernel s and the gluon propagator. The variational equation for the scalar kernel is usually referred to as gap equation. It is highly non-linear and can only be solved numerically. The extension of the ansatz for the quark wave functional with w 0 is not just a quantitative improvement (since the variational space is increased), but it also improves the renormalization procedure, as the linear divergences in the gap equation strictly cancel. Furthermore, the surviving logarithmic divergences always come together with the square of the coupling strength and can thus be absorbed into a scale dependent renormalized effective coupling constant In the variational calculation of the quark sector the non-Abelian Coulomb potential shown in Fig. 2 (b) enters as input. Through the Coulomb string tension σ C , i.e. the coefficient of the asymptotic linear slope of the potential, a scale is inherited from the gluon sector. Choosing σ C = 2σ as suggested by lattice calculations [18] a coupling ofg ( √ σ c ) 3.59 (30) is needed in order to reproduce from the variational solution the phenomenological value of the quark condensate [29] qq = (−235 MeV) 2 .
In Ref. [8] the running coupling constant of Yang-Mills theory was calculated from the ghost-gluon vertex [30]. The result is shown in Fig. 6. From that figure one extracts a running coupling at the scale of the Coulomb string tension ofg which is close to the value given in eq. (30) necessary to reproduce the phenomenological value of the quark condensate. Figure 7 shows the result for the variational kernels v and w. They look quite similar; however, one should notice the different scales. The kernel v is substantially larger than the kernel w. Figure 8 (a) shows the scalar form factor obtained with the coupling constant given in eq. (30) and compared to the corresponding result with the BCS-type wave function where the coupling of the quarks to the spatial gluons is neglected, i.e. eq. (28) with v = w = 0. The latter results in a quark condensate of qq (−165 MeV) 3 , which is substantially smaller than the phenomenological value (31). Finally, Fig. 8 (b) shows the effective quark mass obtained from the full variational calculation and the one from the BCS wave functional. Again the mass is substantially reduced when the coupling to the spatial gluons is ignored.  (16) as input for the gluon energy. Notice that only the section with p = |p| = |q| and z = p · q/pq ist plotted.

Hamiltonian approach to finite-temperature quantum field theory by compactifying a spatial dimension
The variational Hamiltonian approach to QCD in Coulomb gauge can be straightforwardly extended to finite temperatures. For this purpose one uses a variational ansatz for the density operator of the grand canonical ensemble where the exact Hamiltonian is replaced by a single-particle Hamiltonian, with the single-particle energies determined variationally by minimizing the thermodynamic potential or, for vanishing chemical potential, the free energy. This has been done for the Yang-Mills sector in Refs. [9,31]. Here I am going to present a more efficient approach to finite-temperature quantum field theory [33][34][35], which requires no ansatz for the density operator of the grand canonical ensemble. Consider finite-temperature quantum field theory in the standard functional integral approach. Here the finite temperature is introduced by going to Euclidean space and compactifying the Euclidean time dimension by imposing periodic and antiperiodic boundary conditions for Bose and Fermi fields, respectively The length of the compactified dimension L represents then the inverse temperature T −1 = L. One can now exploit the O(4) invariance of the Euclidean Lagrangian to rotate the Euclidean time axis into a space axis and, correspondingly, one space axis into the Euclidean time axis. Of course, thereby all vectorial quantities transform in the same way, i.e. we can choose the transformation: After this rotation we are left with the spatial periodic and antiperiodic boundary conditions As a consequence of the O(4) rotation our spatial manifold is now R 2 × S 1 (L) instead of R 3 while the temporal manifold is R independent of the temperature, i.e. the temperature is now encoded in one spatial dimension while time has infinite extension. We can now apply the usual canonical Hamiltonian approach to this rotated space-time manifold. As the new time axis has infinite extension l → ∞, the partition function is now given by where H(L) is the usual Hamiltonian obtained after canonical quantization, however, now defined on the spatial manifold The full partition function is now obtained from the ground state energy calculated on the spatial manifold R 2 × S 2 (L). Introducing the energy density e(L) on R 2 × S 1 (L) by separating the volume Ll 2 of the spatial manifold from the energy we have It is a little exercise to show that the usual pressure P is given by while the usual energy density ε is obtained as To distinguish this quantity from the (negative) Casimir pressure e(L) eq. (39), which also appears as an energy density in our formalism after the transformation eq. (34), we will denote e(L) as pseudo energy density. Finally, after the O(4) rotation eq. (34), the finite chemical potential μ enters the single-particle Dirac Hamiltonian h in the form where α 3 is the third Dirac matrix and h(μ = 0) the standard Dirac operator coupled to the gauge field. To illustrate the above approach [35] let us first consider a relativistic Bose gas with dispersion relation ω(p) = p 2 + m 2 , where we assume for simplicity a vanishing chemical potential. The usual pressure obtained from the grand canonical ensemble for such a system is given by where n(p) are the finite temperature Bose occupation numbers. On the other hand for the pseudo energy density on the spatial manifold R 2 × S 1 (L) one finds, for the ideal Bose gas with dispersion relation ω(p) = p 2 + m 2 [35] e(L) = 1 2 where p n are the bosonic Matsubara frequencies. This quantity does not look at all like the negative of the pressure (42), as it should by eq. (39). In fact, as it stands it is ill defined: the integral and the sum are both divergent. To make it mathematically well defined, we first use the proper-time regularization of the square root The divergent constant appears because the limit Λ → ∞ of the incomplete Γ-function is not smooth; it drops out when taking the difference to the zero-temperature case after eq. (46) below. With this replacement, the momentum integral in eq. (43) can be carried out in closed form. For the remaining Matsubara sum we use the Poisson resummation formula, after which the proper-time integral can also be carried out, yielding for the pseudo energy density (43) where K ν (z) is the modified Bessel function. The term with n = 0 is divergent and represents the pseudo energy density at zero temperature, which should be eliminated from the pressure. The remaining terms n 0 are all finite and also the remaining sum converges. This sum, however, cannot be carried out analytically for massive bosons (the same applies to the integral in the grand canonical expression (42) for the pressure). In the zero-mass limit we find from eq. (46) for the pressure (39) which is Stefan-Boltzmann law, the correct result also obtained from the grand canonical ensemble. For massive bosons the evaluation of the sum in eq. (46) as well as the evaluation of the integral in eq. (42) have to be done numerically. The result is shown in Fig. 9 (a). As expected the pressure calculated from the compactified spatial dimension reproduces the result of the usual grand canonical ensemble. Figure 9 (b) shows the various contributions to the pressure. It is seen that only a few terms in the sum of eq. (46) are necessary to reproduce the result of the grand canonical ensemble to good accuracy.
In the case of the relativistic Fermi gas with dispersion relation ω(p) = p 2 + m 2 the energy density on R 2 × S 1 (L) is given by where we have now included a non-vanishing chemical potential μ. To make this expression mathematically well-defined one has to resort again to the proper-time regularization and Poisson resummation technique sketched above. The result is Again, the term with n = 0 represents the zero temperature vacuum energy density, which is divergent and has to be removed. As before, this expression can only be calculated in closed form for massless particles. For the remaining sum to converge, an analytic continuation iμL →μ ∈ R is required to carry out the sum ∞ n=1 (−1) n cos(nμ) Continuing back to real chemical potentials one finds through eq. (39) for the pressure which is the correct result obtained also from the usual grand canonical ensemble. In Ref. [36] the above approach was used to study Yang-Mills theory at finite temperature. For this purpose, it is merely required to repeat the variational Hamiltonian approach on the spatial manifold R 2 × S 1 (L). Due to the one compactified spatial dimension the 3-dimensional integral equations of the zero-temperature case are replaced by a set of 2-dimensional integral equations distinguished by different Matsubara frequencies. Below I will use this approach to calculate the effective potential of the Polyakov loop, the order parameter of confinement.

The Polyakov loop
Consider SU(N) gauge theory at finite temperature, where the temperature is introduced by the usual periodic boundary condition in the temporal direction (33). Gauge transformations preserving this boundary conditions need to be periodic only up to an element z of the center Z(N) of the gauge group Since there are N center elements this theory has a residual global Z(N) symmetry, which remains after gauge fixing. However, there are quantities which are sensitive to such a Z(N) symmetry transformation. The most prominent example is the Polyakov loop where A 0 = A a 0 t a is the temporal gauge field in the fundamental representation, and d is the dimension of this representation. A gauge transformation of the form (52) multiplies the Polyakov loop by the center element z P[ The expectation value of the Polyakov loop can be shown to be related to the free energy F ∞ (x) of a static color point charge located at x [37].
In a confining theory this quantity has to be infinite since there are no free color charges, while in a deconfined phase it is finite. Accordingly we find for the expectation value of the Polyakov loop From eq. (54) follows that a state with vanishing expectation value of the Polyakov loop is obviously invariant with respect to the global center transformation, while in the deconfined phase the Z(N) center symmetry is obviously broken. In the continuum theory the Polyakov loop can be most easily calculated in the Polyakov gauge In this gauge one finds, for example, for the SU(2) gauge group that the Polyakov loop is a unique function of the gauge field, at least in the fundamental modular region of this gauge. It can be shown, see Refs. [38], [39], that instead of the expectation value of the Polyakov loop P[A 0 ] one may alternatively use the Polyakov loop of the expectation value, P[ A 0 ], or the expectation value of the temporal gauge field itself, A 0 , as order parameter of confinement. This analysis also shows that the most efficient way to obtain the Polyakov loop is to carry out a so-called background field calculation with a temporal background field a 0 (x) = A 0 (x) chosen in the Polyakov gauge, and then calculate the effective potential e[a 0 ] of that background field. From the minimumā 0 of this potential one evaluates the Polyakov loop P[ A 0 ] = P[ā 0 ], which can then serve as the order parameter of confinement. Such a calculation was done a long time ago in Ref. [40], where the effective potential e[a 0 ] was calculated in 1-loop perturbation theory. The result is shown in Fig. 10 (a). The potential is periodic due to center symmetry. The minimum of the potential occurs at the vanishing background field, which gives P[a 0 = 0] = 1 corresponding to the deconfined phase. This is, of course, expected due to the use of perturbation theory. Below I present the results of a non-perturbative evaluation of e[a 0 ] in the Hamiltonian approach in Coulomb gauge.
At first sight it seems that the Polyakov loop cannot be calculated in the Hamiltonian approach due to the use of the Weyl gauge A 0 = 0. However, we can now use the alternative Hamiltonian approach to finite temperature introduced above, where the temperature is introduced by compactifying a spatial dimension. Here, we compactify the x 3 −axis and consequently put also the background field along this axis a = ae 3 . In the Hamiltonian approach the effective potential of a spatial background field a can be easily calculated by minimizing the expectation value of the Hamiltonian under the constraint A = a. The resulting energy H a = L 2 le(a) is then (up to the spatial volume factor) the effective potential. So the effective potential e(a) is nothing but the pseudo energy density considered earlier, but now calculated in a background gauge with the contraint A = a.

The effective potential of the Polyakov loop
After lengthy calculations exploiting the gluon gap equation (14) one finds for the effective potential of the Polyakov loop the following expression e(a, L) = Here ω(p) is the gluon energy and χ(p) is the ghost loop. Furthermore, these quantities have to be taken with the momentum variable  where p ⊥ is the momentum corresponding to the two uncompactified space dimensions while p n = 2πn/L is the Matsubara frequency resulting from the compactification of the third dimension. Furthermore, σ · a ≡ σ b a b denotes the product of the color background field with the root vectors σ b of the gauge group. Equation (59) includes also the summation over the roots σ of the gauge group. In Ref. [33,34] the effective potential (59) was explicitly calculated using for ω(p) and χ(p) the results from the variational calculation in Coulomb gauge at zero temperature [8]. This represents certainly an approximation since, in principle, one should use the finite-temperature solutions obtained in Ref. [36].
Before I present the full results let me ignore the ghost loop χ(p) in eq. (59) and consider the ultraviolet and infrared limit of the gluon energy. If we choose the ultraviolet limit ω(p) = p, we obtain from eq. (59) with χ(p) = 0 precisely the Weiss potential, shown in Fig. 10 (a), which corresponds to the deconfined phase. Choosing for the gluon energy its infrared limit ω(p) = M 2 /p one finds from eq. (59) with χ(p) = 0 the (center symmetric) potential shown in Fig. 10 (b). From its center symmetric minimumā = π/L one finds a vanishing Polyakov loop P[ā] = 0 corresponding to the confined phase. Obviously, the deconfining phase transition results from the interplay between the confining infrared and the deconfining ultraviolet potentials. Choosing for the gluon energy the sum of the UV-and IR-parts ω(p) = p + M 2 /p, which can be considered as an approximation to the Gribov formula (16), one has to add the UV and IR potentials and finds a phase transition at a critical temperature T c = √ 3M/π. With the Gribov mass M ≈ 880 MeV this gives a critical value of T c ≈ 485 MeV for the color group SU(2), which is much too high as compared to the lattice value of 312 MeV [32]. One can show analytically [33,34] that the neglect of the ghost loop χ(p) = 0 shifts the critical temperature to higher values. If one uses for the gluon energy ω(p) the Gribov formula (16) and includes the ghost loop χ(p) one finds the effective potential shown in Fig. 11 (a), which shows a second order phase transition and gives a transition temperature of T c ≈ 269 MeV for the gauge group SU (2), which is in the right ballpark. The Polyakov loop P[ā] calculated from the minimumā of the effective potential e(a, L) (59) is plotted in Fig. 12(a) as function of the temperature.
The effective potential for the gauge group SU(3) can be reduced to that of the SU(2) group by noticing that the SU(3) algebra consists of three SU(2) subalgebras characterized by the three positive The resulting effective potential for SU(3) is shown in Fig. 13 as function of the components of the background field in the Cartan algebra a 3 , a 8 . Above and below T c the absolute minima of the potential occur in both cases for a 8 = 0. Cutting the 2-dimensional potential surface at a 8 = 0 one finds the effective potential shown in Fig. 11 (b), which shows a first order phase transition with a critical temperature of T c ≈ 283 MeV. The first order nature of the SU(3) phase transition is also seen in Fig. 12 (b), where the Polyakov loop P[ā] is shown as function of the temperature.

Conclusions
In this talk I have shown that the Hamiltonian approach to QCD in Coulomb gauge gives a decent description of the infrared properties of the theory and at the same time can be straightforwardly  extended to finite temperatures, where it yields critical temperatures for the deconfinement phase transition in the right ballpark. Furthermore, the approach has also produced the correct order of the deconfinement phase transition, viz. first order for SU(3) and second order for SU (2). The obtained results are very encouraging and call for an extension of the present approach to non-zero chemical potentials.