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Thermal effect in hot QCD matter in strong magnetic fields

Xin-Jian Wen and Jia Zhang Institute of Theoretical Physics, State Key Laboratory of Quantum Optics and Quantum Optics Devices, Shanxi University, Taiyuan, Shanxi 030006, China
Abstract

The quasiparticle model is improved by the free magnetic contribution to investigated the QCD matter in a strong magnetic field. The temperature-dependent bag function is determined by the thermodynamic consistency to represent the difference in energy density between physical vacuum and lowest state of QCD. It is found that the positive bag function vanishes at high temperature indicating the deconfinement. The rapid decrease of the bag function in stronger magnetic fields reveals the so-called inverse magnetic catalysis. The interaction measure at high temperature remains so large that the usual Stefan-Boltzmann limit can not be reached. We suggest a limit |qiBm|T2/4|q_{i}B_{m}|T^{2}/4 for each landau level pressure. Finally, it is demonstrated that the positive magnetization modified by the bag function and free magnetic contribution indicates the paramagnetic characteristic of QCD matter.

I Introduction

It has been observed that the strongly interacting matter, quark-gluon plasma (QGP), produced in the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC) behaves more like a near-perfect fluid. The QCD theory in the magnetic background may reveal a better understanding of the QGP that have rich collective effects Lai:2000at ; Koothottil:2020riy . Many efforts have been done in theoretical work revealing interesting properties of strongly interacting matter in the strong magnetic field Andersen:2014xxa ; Miransky:2015ava . With the development of relativistic heavy ion collisions, the study of medium effect of quark-gluon plasma becomes more active. Quark self-energy at high temperature receives the contribution of both the electric scale and magnetic scale, which have profound impact of confinement effects on thermal quark collective excitation Su:2014rma ; Jamal:2017dqs .

In hot dense quark matter, one of the most important medium effects is the effective mass generated by the nonperturbative interaction of the particles with the system. In literature, the phenomenological models overcome the difficulty of the QCD theory at finite temperature and/or chemical potentials. A natural mechanism for quark confinement is given by the MIT bag model DeTar:1983rw . The bag model was proposed to explain hadrons and quark confinement, which artificially constrains the quarks inside a finite region in space. However, the bag model is not able to well exhibit the phase transition of the deconfinement. The quark quasiparticle model, as an extended bag model, has been developed in studying the bulk properties of the dense quark matter at finite density and temperature QPM ; Thaler:2003uz ; Schertler:1996tq ; He:2023gva and the strangeles in finite size Wen:2009zza . The quasiparticle description has been assumed to be valid also in the case of sufficiently high temperature Gorenstein:1995vm ; Peshier:1995ty ; Levai:1997yx . The advantage of the quasiparticle model is the introduction of the medium-dependent quark mass scale to reflect the nonperturbative QCD properties Srivastava:2010xa and color confinement mechanism Schneider:2001nf . The transport properties of the quark gluon plasma have been well investigated by the noninteracting/weakly interacting particles with effective masses Albright:2015fpa . The hard thermal loop(HTL) approximation can also be used to calculate the effective quark mass, but these calculations are valid only in the perturbative regime of QCD Bellac:2011kqa ; Peshier:2002ww ; Levai:1997yx . There are also self-consistent quasiparticle models and single parameter quasiparticle model Koothottil:2018akg ; Bannur:2010zz ; Bannur:2007tk . The medium effects are taken into account by considering quarks and gluons as quasiparticles. Their temperature dependent masses are proportional to the plasma frequency. More recent developments have shown that quasiparticles with effective fugacity have been successful in describing the lattice QCD results Chandra:2009jjo ; Chandra:2011en , which was initially proposed by Chandra and RavishankarChandra:2011en ; Chandra:2007ca .

It is well known that quarks are bound inside hadron through strong interaction, and it has not yet been found that quarks can exist independently. Based on this fact, the nature of quark confinement was derived. According to lattice simulations, the deconfinement phase transition is of first order Boyd:1996bx . In some phenomenological models, an order parameter of the deconfinement transition is the Polyakov loop which is the trace of a Wilson line along a closed loop in the time directionLi:2018ygx . For the SU(3) pure gauge theory, the deconfined phase transition at high temperature corresponds to the spontaneous Z(3) symmetry breaking. However, the study of symmetry can be complicated in QCD due to the quark dynamics. In particular, the quark confinement and vacuum energy density can be well described by the density-dependent bag constant Goloviznin:1992ws ; Srivastava:2010xa ; Thaler:2003uz . In the present work, the formula of QGP has been described as a non-interacting gas of quarks at zero chemical potential but finite temperature, taking into account the phenomenological bag constant. As for gluon gas, the equation of state for gluons has been excellently described using the ideal gas approximation at high temperatures in lattice calculations Peshier:1994zf ; Peshier:1995ty .

The paper is organized as follows. In Section II, we present the thermodynamics of the magnetized QGP in the quasiparticle model. In Section III, the numerical results for the confinement bag function and the thermodynamic quantities in the strong magnetic field at finite temperatures. The last section is a short summary.

II Thermodynamics of quasiparticle model in strong magnetic fields

The important feature of the quasiparticle model is the medium dependence of quark masses in describing QCD nonperturbative properties. The quasiparticle quark mass is derived at the zero-momentum limit of the dispersion relations from an effective quark propagator by resuming one-loop self-energy diagrams in the hard dense loop (HDL) approximation. The dynamical information for gluonic degrees of freedom can also be accessed through the effective gluon mass. In this paper, the effective quark mass mqm_{q} and gluon mass mgm_{g} are adopted as Levai:1997yx ; Pisarski:1989cs ; Plumari:2011mk

mg(T)\displaystyle m_{g}(T) =\displaystyle= 16(Nc+12Nf)g2T2,\displaystyle\sqrt{\frac{1}{6}(N_{c}+\frac{1}{2}N_{f})g^{2}T^{2}}\,, (1)
mq(T)\displaystyle m_{q}(T) =\displaystyle= 12(mi0+mi02+Nc212Ncg2T2),\displaystyle\frac{1}{2}\big{(}m_{i0}+\sqrt{m_{i0}^{2}+\frac{N_{c}^{2}-1}{2N_{c}}g^{2}T^{2}}\big{)}\,, (2)

where mi0m_{i0} denotes the quark current mass of the quark flavor ii. The constant gg is the strong interaction coupling. In order to reflect the asymptotic freedom of QCD, one can also use a running coupling constant g(Q/Λ)g(Q/\Lambda) in the equations of state of strange matter Shirkov:1997wi . The parameterization of the coupling as a function of temperature close to the theory is adopted as Peshier:1994zf

g2(T,Tc)=48π2(11Nc2Nf)ln(λ2(T/TcTs/Tc)2)(ΛTcT)η.\displaystyle g^{2}(T,T_{c})=\frac{48\pi^{2}}{(11N_{c}-2N_{f})\ln(\lambda^{2}(T/T_{c}-T_{s}/T_{c})^{2})}(\frac{\Lambda T_{c}}{T})^{\eta}. (3)

The current mass can be neglected for up and down quarks, while the strange quark is taken to be massive. Because the vanishing current mass is assumed for up and down quarks, Eq. (2) is reduced to the simple form

mu,d=13gT.\displaystyle m_{u,d}=\frac{1}{\sqrt{3}}gT. (4)

As a typical treatment in the quasiparticle model, one implements confinement by introducing a bag pressure, measuring the level difference between the physical vacuum and the ground state in the colorful world of QCD Castorina:2011ja . To account for the essential non-perturbative features, the corresponding thermodynamics is based on the ideal gas partition function with additional contributions,

TlnZ=Tln(Z0ZvacZmag),\displaystyle T\ln Z=T\ln(Z_{0}Z_{\mathrm{vac}}Z_{\mathrm{mag}}), (5)

where the vacuum partition depends on the bag function TlnZvac=B(T)VT\ln Z_{\mathrm{vac}}=-B(T)V Castorina:2011ja and the term ZmagZ_{\mathrm{mag}} stands for the free magnetic field contribution. The conventional matter contribution is introduced by Z0Z_{0}. So the total partition function can produce the thermodynamic quantities from the self-consistent relation. Within the framework of the temperature-dependent mass m(T)m(T), the pressure of the system is expressed as

P(T,Bm)=TVlnZ(T,Bm)=i=q,g[Ωi(T,Bm)+Bi(T,Bm)]B0𝒱(T0,Bm).\displaystyle P(T,B_{m})=\frac{T}{V}\ln Z(T,B_{m})=-\sum_{i=q,g}[\Omega_{i}(T,B_{m})+B_{i}(T,B_{m})]-B_{0}-{\cal V}(T_{0},B_{m}). (6)

The first term Ωi\Omega_{i} is the conventional matter contribution. The bag constant B0B_{0} stands for the vacuum energy density at zero temperature. The variant term Bi(T,Bm)B_{i}(T,B_{m}) resembles the interaction term from quasiparticles and can be interpreted as the thermal vacuum energy density. We assume Maxwell term 𝒱(T0,Bm){\cal V}(T_{0},B_{m}) is independent on the quark mass but on the magnetic field, which represent the free pressure of magnetic contribution Menezes:2008qt ; Mizher:2010zb ; Fraga:2012fs

𝒱(T0,Bm)=i=qNc|eiBm|22π2[ζ(1,xi)ζ(1,0)12(xi2xi)ln(xi)+xi24],\displaystyle{\cal V}(T_{0},B_{m})=-\sum_{i=q}\frac{N_{c}|e_{i}B_{m}|^{2}}{2\pi^{2}}\left[\zeta^{\prime}(-1,x_{i})-\zeta^{\prime}(-1,0)-\frac{1}{2}(x_{i}^{2}-x_{i})\ln(x_{i})+\frac{x_{i}^{2}}{4}\right], (7)

where the parameter xi=mi2/(2|qiBm|)x_{i}=m_{i}^{2}/(2|q_{i}B_{m}|) is defined at the moderate temperature T0=150T_{0}=150 MeV in the thermal bag. The constant ζ(1,0)=0.165421\zeta^{\prime}(-1,0)=-0.165421... was introduced in Ref Fraga:2012fs , which is helpful to maintain a positive magnetic pressure. The presence of 𝒱(T0,Bm){\cal V}(T_{0},B_{m}) would not change the thermodynamically self-consistent relation P/mi=0\partial P/\partial m_{i}=0 in quasiparticle model. So we have the following differential equation

dBidTdTdmi=Ωimi.\displaystyle\frac{dB_{i}}{dT}\frac{dT}{dm_{i}}=-\frac{\partial\Omega_{i}}{\partial m_{i}}. (8)

So the temperature dependent term Bi(T,Bm)B_{i}(T,B_{m}) is

Bi(T,Bm)=0TΩimidmidT𝑑T.\displaystyle B_{i}(T,B_{m})=-\int_{0}^{T}\frac{\partial\Omega_{i}}{\partial m_{i}}\frac{dm_{i}}{dT}dT. (9)

The derivative Ωi/mi\partial\Omega_{i}/\partial m_{i} is

Ωimi=di|eiBm|π2ν=0(2δν0)0f(εi)miεi𝑑pz.\displaystyle\frac{\partial\Omega_{i}}{\partial m_{i}}=\frac{d_{i}|e_{i}B_{m}|}{\pi^{2}}\sum_{\nu=0}^{\infty}(2-\delta_{\nu 0})\int_{0}^{\infty}f(\varepsilon_{i})\frac{m_{i}}{\varepsilon_{i}}dp_{z}. (10)

where the fermion distribution function is f(εi)=1/(1+exp(εiT))f(\varepsilon_{i})=1/({1+\exp(\frac{\varepsilon_{i}}{T})}) and the single particle energy is εi=pz2+mi2+2νeiBm\varepsilon_{i}=\sqrt{p_{z}^{2}+m_{i}^{2}+2\nu e_{i}B_{m}} due to the quantization of orbital motion of charged particles in the presence of a strong magnetic field along the zz axis Chakrabarty:1996te . The derivative of the mass m(T)m(T) with respect to the temperature is

dmidT=Nc214Ncg2Tm02+(Nc21)g2T2/(2Nc)+mig2g2T,\displaystyle\frac{dm_{i}}{dT}=\frac{N_{c}^{2}-1}{4N_{c}}\frac{g^{2}T}{\sqrt{m_{0}^{2}+(N_{c}^{2}-1)g^{2}T^{2}/(2N_{c})}}+\frac{\partial m_{i}}{\partial g^{2}}\frac{\partial g^{2}}{\partial T}, (11)

which will be simplified as dmidT=g3\frac{dm_{i}}{dT}=\frac{g}{\sqrt{3}} for zero current mass and the constant coupling gT=0\frac{\partial g}{\partial T}=0. If one takes into account the running coupling g(T)g(T), the derivative of the mass mi(T)m_{i}(T) with respect to the TT should be calculated through the full differential relation.

The entropy density, as a measure of phase space, is unaffected by Bi(T,Bm)B_{i}(T,B_{m}) Thaler:2003uz , which is clearly understood from the relation (8). Similar to the number density, the entropy density is written based on the fundamental thermodynamic relation,

si=ΩiT=di|eiBm|π2ν=0(2δν0)0f(εi)p2+εi2Tεi𝑑pz.\displaystyle s_{i}=-\frac{\partial\Omega_{i}}{\partial T}=\frac{d_{i}|e_{i}B_{m}|}{\pi^{2}}\sum_{\nu=0}^{\infty}(2-\delta_{\nu 0})\int_{0}^{\infty}f(\varepsilon_{i})\frac{p^{2}+\varepsilon_{i}^{2}}{T\varepsilon_{i}}dp_{z}. (12)

The net effect of the bag function is to cancel the entropy density contribution, which would arise from the dependence of the mass m(T)m(T) on the temperature. It is well known to us that the energy density and pressure should vanish in vacuum. So the pressure should be normalized by requiring zero pressure at zero temperature as

Peff(T,Bm)=P(T,Bm)P(0,Bm).\displaystyle P^{\mathrm{eff}}(T,B_{m})=P(T,B_{m})-P(0,B_{m}). (13)

The magnetization is an important thermodynamic quantity in understanding the QCD matter Ferrer:2019xlr . The development of the study on the magnetization in various methods has been summarized in Ref. Cao:2023bmk . At zero temperature, the magnetization is found to be positive and to be responsible for the anisotropic pressures Felipe:2007vb ; Strickland:2012vu . We propose the expression of the magnetization in quasiparticle model as,

=PeffBm=i=u,d,s(ΩiBm+BiBm+𝒱iBm),\displaystyle{\cal{M}}=\frac{\partial P^{\mathrm{eff}}}{\partial B_{m}}=-\sum_{i=u,d,s}\left(\frac{\partial\Omega_{i}}{\partial B_{m}}+\frac{\partial B_{i}}{\partial B_{m}}+\frac{\partial{\cal V}_{i}}{\partial B_{m}}\right), (14)

where the first term is the conventional contribution from the pure quasiparticle Menezes:2015fla . The second term demonstrates that the effective bag function would have additional contribution to the magnetization, which reveals the medium effect on the hot quark matter. It can be written as,

BiBm=Nc|ei|miπ2ν=0(2δν0)0f(εi)(νBmε2+f(εi)ν|ei|BmεiT1)dpzεi.\displaystyle\frac{\partial B_{i}}{\partial B_{m}}=\frac{N_{c}|e_{i}|m_{i}}{\pi^{2}}\sum_{\nu=0}^{\infty}(2-\delta_{\nu 0})\int_{0}^{\infty}f(\varepsilon_{i})\left(\frac{\nu B_{m}}{\varepsilon^{2}}+f(\varepsilon_{i})\frac{\nu|e_{i}|B_{m}}{\varepsilon_{i}T}-1\right)\frac{dp_{z}}{\varepsilon_{i}}. (15)

III Numerical result and conclusion

In the framework of the preceding quasiparticle model, we have done the numerical calculations with the quark current mass values mu=mdm_{u}=m_{d}= 0, and msm_{s}=120 MeV. The constant term B0B_{0} is (145MeV)4(145\mathrm{MeV})^{4}. The effective bag constant acts as an energy penalty for the deconfined phase. In Fig. 1, the effective bag constant B(T,Bm)B(T,B_{m}) is shown as a function of the temperature at different magnetic fields Bm=0.2B_{m}=0.2, 0.4, 0.6 GeV2. It falls to zero at high temperature, which means that the deconfined state has larger pressure and is energetically preferred. Compared with the fixed coupling constant g=3g=3, the running coupling constant g(T)g(T) leads to a decrease of B(T,Bm)B(T,B_{m}) at higher temperature. The increase of the magnetic field will not change the vacuum energy B(T,Bm)B(T,B_{m}) at T=0T=0. But the decrease of the bag constant would be more rapidly in stronger magnetic fields, which indicates a lower value of the critical temperature for the deconfinement transition.

Refer to caption
Figure 1: The effective bag function B(T,Bm)B(T,B_{m}) is shown as functions of temperatures denoting the deconfinement transition. The B(T,Bm)B(T,B_{m}) decreases more rapidly with increasing temperatures at stronger magnetic fields for both constant coupling and running coupling constants.

In the quasiparticle model, the decrease of the effective bag constant B(T,Bm)B(T,B_{m}) denotes the deconfinement transition. The critical temperature can be determined by the position of half-height of the bag constant. In Fig. 2, the pseudocritical temperature is plotted by the red solid curve. For the convenience of comparison, the result from PNJL is marked by the black dashed curve Tavares:2021fik . It can be clearly seen that the trend of the decrease of the TpcT_{pc} with the magnetic field is close to the LQCD result marked by the shadow band in the panel Bali:2011qj . Moreover, the pseudocritical temperature decreases by about 10 percent of its original value at zero magnetic field. Our result is in agreement with the so-called inverse magnetic catalysis effect revealed by the LQCD.

Refer to caption
Figure 2: The pseudocritical temperature for the deconfinement transition in quasiparticle model (red curve) compared with the results of the PNJL model (dashed curve) Tavares:2021fik and of LQCD (shadow band )Bali:2011qj .

Fig. 3 illustrates how the pressure and the energy density (in unit of T4T^{4}) depend on the temperature of the medium. In the region around and just above the critical temperature, the energy density rises much more rapidly than the pressure, which gives rise to a observed rapid increase of the interaction measure. At stronger magnetic fields, the larger pressure and energy density are obtained at the high temperature. However, the temperature is not the only scale with the dimension of the energy. The pressure as well as the energy density can not asymptotically converge to their Stefan-Boltzmann value PSB/T4=P^{\mathrm{SB}}/T^{4}=constant at TT\rightarrow\infty. The deviations from the usual Stefan-Boltzmann values are due to the quarks are constrained by the landau level in strong magnetic fields.

Refer to caption
Figure 3: The scaled pressure Peff/T4P^{\mathrm{eff}}/T^{4} on left panel and energy density ϵ/T4\epsilon/T^{4} on right panel are always increasing functions of the temperature. It is apparent that the Stefan-Boltzmann (S-B) limit is absent at high temperatures in strong magnetic fields.

Interaction measure is the trace of energy-momentum tensor. For non-interacting massless constituents (the “conformal” limit), is zero, so that the temperature is the only scale. In a strong magnetic field, the interaction measure is defined as Δ(T)(ε3P)/T4\Delta(T)\equiv(\varepsilon-3P)/T^{4} for quark gluon plasma. In Fig. 4, the trace anomaly of the energy momentum tensor is plotted as a function of temperature. The so-called interaction measure normalized by T4T^{4} gives the deviation from the free gas relation between the energy density and the pressure and is also a measure of the breakdown of conformal symmetry. Even though the temperature dependent coupling constant is employed to realize the asymptotic freedom at high temperature, the non-zero value indicates that some interactions must still be present due to the landau levels in magnetic fields. The Δ(T)\Delta(T) at high temperature will remain larger at stronger magnetic fields, which is in agreement with LQCD that the interaction measure remains large even at very high temperatures, where the Stefan-Boltzmann (S-B) limit is not yet reached.

Refer to caption
Figure 4: The interaction measure is shown as functions of the temperatures in different magnetic fields. It remains so larger at high temperatures that the interaction must be still present at eBm=0.6eB_{m}=0.6 GeV2 marked by the solid curve.

In fact, the S-B limit for the the nn-th landau level can be defined as,

PSB(n)|qiBm|T2=14.\displaystyle\frac{P^{\mathrm{(n)}}_{\mathrm{SB}}}{|q_{i}B_{m}|T^{2}}=\frac{1}{4}. (16)

In Fig. 5, the pressures and entropy of ii-flavor quarks in the nn-th Landau level are shown as the function of temperatures. At sufficiently high temperatures, the scaled pressure P(n)/(|qiBm|T2)P^{(n)}/(|q_{i}B_{m}|T^{2}) on the left panel can approach the limit marked by the dash-dotted horizontal line. In particular, the pressure from the lowest landau level (n=0) marked by the solid line is close to the S-B limit line. Moreover, much higher temperature is required for any excited levels (n=1, 2) to reach the limit. It can be accounted for by the fact that the higher level leads to the larger effective mass and therefore results in a larger deviation from the S-B limit. Correspondingly, the entropy S(n)/(|qiBm|T)S^{(n)}/(|q_{i}B_{m}|T) in the nn-level has the S-B limit on right panel in the strong magnetic field.

Refer to caption
Figure 5: The scaled pressure and entropy of ii-flavor quarks lying in Landau levels n=0n=0 , 1 and 2. At high enough temperatures, the three lines approach the Stefan-Boltzman limit marked by the dash-dotted horizontal line. It is characteristic that the limit is early approached in the lowest landau level.

In Fig. 6, the magnetization of strange quark matter is shown as a function of the temperature at fixed magnetic fields eBm=0.2eB_{m}=0.2, 0.4, 0.6 GeV2 marked by the black, red, and blue solid curves, respectively. The positive value produces the paramagnetic characteristic for the whole temperature range Bali:2013owa . The magnetization increases with increasing temperature at fixed magnetic fields. It can be understood that the more Landau levels at high temperature the stronger the magnetization. The effective bag function marked by the red dotted line enhances the magnetization at finite temperature. The discrepancy of the magnetization at low temperature is sizable due to the free magnetic contribution. By comparison with the lattice result marked by the scattering triangles at eBm=0.2eB_{m}=0.2 and 0.4 GeV2 Bali:2014kia , it can be concluded that the ascending trend and the magnetic effect are consistent. In particular, increase of the magnetic field enhances the magnetization of the quark matter.

Refer to caption
Figure 6: The magnetization of the strange quark matter is shown as a function of the temperature at eBm=0.2eB_{m}=0.2, 0.4, 0.6 GeV2. The LQCD result at eBm=0.2eB_{m}=0.2 and 0.4 GeV2 is marked by scattering triangles for comparison Bali:2014kia .

IV Summary

In this paper, we have investigated the hot QCD matter exposed to sufficiently high magnetic fields, which could be generated in RHIC experiments. The quasiparticle model is extended by including the free magnetic contribution and the effective thermomagnetic bag constant, which is self-consistent derived to represent the confinement. The running coupling constant has been employed to reflect the asymptotic freedom of QCD. It has been found that the decrease of the effective bag constant at the high temperature indicates the occurence of the deconfinement transition. Moreover, the stronger magnetic field results in a more rapidly decrease of the effective bag constant, which provides a novel method to account for the so-called inverse magnetic catalysis effect. Moreover, the paramagnetic characteristic of QCD is obtained in the quasiparticle model. The effective bag constant would have an additional contribution in the new definition of the magnetization due to the medium effect. It is concluded that the magnetization modified by the function and free magnetic contributions can only account for the trend revealed by the lattice result. It would be of some interest to improve the quasiparticle model to quantitatively interpret the lattice results in future.

For the quark-gluon plasma in strong magnetic field, the interaction measure remains larger even at very high temperature and indicates some interactions are present. Therefore, the usual S-B limit is not applicable. The deviation form the S-B limit becomes remarkable with the massive effective mass led by the stronger magnetic field. Not only the temperature but also the magnetic field are the scale of energy. We suggested that for single landau level, the S-B limit of the quark pressure can be defined as |qiBm|T2/4|q_{i}B_{m}|T^{2}/4. It has been shown that the lowest landau level is close to the S-B limit, while higher temperature is required for the excited levels to approach the limit.

Acknowledgements.
The authors would like to thank support from the National Natural Science Foundation of China under the Grant Nos. 11875181, 12047571, and 11705163. This work was also sponsored by the Fund for Shanxi ”1331 Project” Key Subjects Construction.

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