Charged rho superconductor in the presence of magnetic field and rotation

Abstract

In this work, we mainly explore the possibility of charged rho (\(\rho ^\pm \)) superconductor in the presence of parallel magnetic field and rotation within three-flavor Nambu–Jona-Lasino model. By following similar schemes as in the previous studies of charged pion (\(\pi ^\pm \)) superfluid, the \(\rho ^\pm \) superconductor is found to be favored for both choices of Schwinger phase in Minkowski and curved spaces. Due to the stability of the internal spin structure, charged rho begins to condensate at a smaller threshold of angular velocity than charged pion for the given large magnetic fields. Even the axial vector meson condensation is checked – the conclusion is that \(\rho ^\pm \) superconductor is the robust ground state at strong magnetic field and fast rotation, which actually sustains to very large angular velocity.

Introduction

Nowadays, several extraordinary conditions can be realized in the terrestrial relativistic heavy ion collisions (HICs), such as strong electromagnetic (EM) field [1,2,3,4] and fast rotation [5,6,7]. Under such circumstances, the properties of quantum chromodynamics (QCD) system are quite interesting and attractive topics. Actually, magnetic field and rotation share some similar effect, thus the proposal of chiral magnetic effect is right followed by that of chiral vortical effect around 2008. These anomalous transport phenomena were intensively studied since then [8,9,10], and recently a very important breakthrough has been acheived in the BES II experiment of STAR group [11]. Nevertheless, along with the discoveries of magnetic catalysis effect at zero temperature [12, 13] and global polarization of \(\Lambda \) hyperon in peripheral HICs [14,15,16], some unexpected features emerge and still require proper explanations: the inverse magnetic catalysis effect [18, 19] and the “sign puzzles” of the local polarizations [16, 20,21,22,23]. In some sense, the extreme conditions open a wide realm for the searching of new phases, such as \(\rho ^\pm \) superconductor in pure magnetic field [24, 25], neutral pseudoscalar superfluid in parallel EM field [26,27,28,29] and \(\pi ^\pm \) superfluid in parallel magnetic field and rotation (\(\mathbf{B}\parallel \varvec{\Omega }\)) [30]. Among others, the possibility of \(\rho ^\pm \) superconductor was under fierce debate since its proposal  [24, 25, 31,32,33,34,35,36], mainly concerning the internal quark-antiquark effect on rho mesons.

Actually, in peripheral HICs, the generated magnetic field in and global rotation of the fireball are roughly along the same direction [2, 7], which naturally imposes theorists an urgent mission to clarify the ground state of QCD in such circumstance. Regard to the existence of \(\pi ^\pm \) superfluid in \(\mathbf{B}\parallel \varvec{\Omega }\), it is controversial according to the studies in Nambu–Jona-Lasinio (NJL) model, where one is immersed in the ambiguity of the definition for Schwinger phase [37, 38]. In pure magnetic field, the Schwinger phase is just the gauge dependent part of the meson propagator; but with rotation presented, we are not able to find a consistent one for all Landau levels – that causes somewhat arbitrariness. The breaking effect of rotation on the internal spin structure of charged pion was checked in these works for choices of Schwinger phase (SP) in Minkowski and curved spaces, respectively. It turned out that \(\pi ^\pm \) superfluid is never favored for SP in curved space and only favored in the intermediate regime of angular velocity for SP in Minkowski space [38]. As mentioned in the conclusion of Ref. [37], the spins of valence quark and antiquark are along the same direction in rho vector mesons; thus, the spin-up \(\rho ^+\) meson is stable in the presence of either strong magnetic field B or large rotating angular velocity \(\Omega \) along z direction. Due to the mass reduction in B and effective isospin chemical potential generated by \(\Omega \), it is quite probable that \(\rho ^\pm \) superconductor would occur in \(\mathbf{B}\parallel \varvec{\Omega }\) and keep robust to very fast rotation. Once verified, we are more able to figure out the true phase diagram of QCD in \(\mathbf{B}\parallel \varvec{\Omega }\).

Similar to the electric field discussed in Ref. [26], the rotation term breaks the semi-positivity of fermion determinante in the partition function. Therefore, the study in such setup is free from the constraint of Vafa-Witten (VW) theorem [33, 39], which was previously adopted as the main point against \(\rho ^\pm \) superconductor in pure magnetic field. To show the importance of rotation effect on \(\rho ^\pm \) superconductor, we’d like to mention the interesting results found in Ref. [40]: At finite isospin chemical potential \(\mu _I\), \(\pi ^\pm \) superfluid is always favored over \(\rho ^\pm \) superconductor; but \(\rho ^\pm \) superconductor would finally manage to overwhelm \(\pi ^\pm \) superfluid with \(\Omega \) increasing.

After getting some intuitions from the Weinberg model in Sect. 2, the paper keeps a similar structure as our previous work Ref. [37]. In Sect. 3, we present the formalism for SU(3) NJL model in rotating frame with a parallel magnetic field, where the simplest forms of vector interactions are introduced to explore rho meson physics [35]. Then, the quadratic coefficient in Ginzburg-Landau expansion will be evaluated analytically in Sect. 4 with the choice of SP in Minkowski space in Sect. 4.1 and of SP in curved space in Sect. 4.2, respectively. Eventually, the numerical results will be illuminated in Sect. 5 to check the stability of QCD system against \(\rho ^\pm \) superconductor and we give a simple conclusion in Sect. 6. The natural units \(c=\hbar =k_{\mathrm{B}}=1\) are used throughout.

Intuitions from Weinberg model

From the chiral effective Weinberg model [41] with pion and rho mesons the fundamental degrees of freedom, the Lagrangian density can be extended to the case with \(\mathbf{B}\parallel \varvec{\Omega }\) ias

$$\begin{aligned} \mathcal{L}= & {} {1\over 2}\left( {(D_\mu \varvec{\pi })^\dagger \cdot D^\mu \varvec{\pi }\over (1+{\varvec{\pi }^\dagger \cdot \varvec{\pi }\over f_\pi ^2})^2}-{m_\pi ^2\,\varvec{\pi }^\dagger \cdot \varvec{\pi }\over 1+{\varvec{\pi }^\dagger \cdot \varvec{\pi }\over f_\pi ^2}}\right) -{1\over 4} \varvec{\rho }_{\mu \nu }^\dagger \cdot \varvec{\rho }^{\mu \nu }\nonumber \\&+{m_\rho ^2\over 2}\left[ \varvec{\rho }_\mu \!+\!{g_\rho \varvec{\pi }\!\times \! D_\mu \varvec{\pi }\over m_\rho ^2(1\!+\!{\varvec{\pi }^\dagger \cdot \varvec{\pi }\over f_\pi ^2})}\right] ^\dagger \cdot \left[ \varvec{\rho }^\mu \!+\!{g_\rho \varvec{\pi }\!\times \! D^\mu \varvec{\pi }\over m_\rho ^2(1\!+\!{\varvec{\pi }^\dagger \cdot \varvec{\pi }\over f_\pi ^2})}\right] \nonumber \\&\pm i{e\over 2}F^{\mu \nu }{\rho }_\mu ^\mp {\rho }_\nu ^\pm -{B^2\over 2}, \end{aligned}$$
(1)

where chiral symmetry is nonlinearly realized through the term \(1+{\varvec{\pi }^\dagger \cdot \varvec{\pi }\over f_\pi ^2}\) in the denominators, and magnetic and rotation effects are encoded in the covariant derivative \(D_\mu \). Neglecting all the self-interactions of pions for simplicity, the Lagrangian density is then reduced to

$$\begin{aligned} \mathcal{L}= & {} -{B^2\over 2}+{1\over 2}\left[ {(D_\mu \varvec{\pi })^\dagger \cdot D^\mu \varvec{\pi }}-{m_\pi ^2\,\varvec{\pi }^\dagger \cdot \varvec{\pi }}\right] -{1\over 4} \varvec{\rho }_{\mu \nu }^\dagger \cdot \varvec{\rho }^{\mu \nu }\nonumber \\&+{m_\rho ^2\over 2}\varvec{\rho }_\mu ^\dagger \cdot \varvec{\rho }^\mu \pm i{e\over 2}F^{\mu \nu }{\rho }_\mu ^\mp {\rho }_\nu ^\pm +{g_\rho \over 2}\left[ \varvec{\rho }_\mu ^\dagger \cdot ({\varvec{\pi }\times D^\mu \varvec{\pi }})\right. \nonumber \\&\left. +(\varvec{\pi }\times D_\mu \varvec{\pi })^\dagger \cdot \varvec{\rho }^\mu \right] . \end{aligned}$$
(2)

Here, the isovectors are defined in the electric charge eigenstates: \(\varvec{\pi }=(\pi ^0,\pi ^-,\pi ^+)\) and \(\varvec{\rho }=(\rho ^0,\rho ^-,\rho ^+)\), and we assume for convenience that the rho vector mesons are in the spin eigenstates: \(\rho _\mu =(\rho _t,\rho _\downarrow ,\rho _0,\rho _\uparrow )\). Take \(\rho \) mesons for example, the charge eigenstates are related to the isospin ones \(\rho ^{i}\ (i=1,2,3)\) as

$$\begin{aligned} \rho ^0=\rho ^3,\ \rho ^\pm ={\rho ^1\mp i\rho ^2\over {\sqrt{2}}}, \end{aligned}$$

and the spin eigenstates are defined by the Lorentz components \(\rho _\mu \ (\mu =t,x,y,z)\) as

$$\begin{aligned} \rho _0=\rho _z,\ \rho _{\uparrow /\downarrow }={\rho _{x}\mp i\,\rho _{y}\over \sqrt{2}}. \end{aligned}$$

In the vacuum, the strength tensors of \(\rho \) mesons are defined in a similar way as those of gauge fields in the SU(2) Yang-Mills theory:

$$\begin{aligned} {\rho }_{\mu \nu }^a\equiv \partial _\mu {\rho }_{\nu }^a-\partial _\nu {\rho }_{\mu }^a+g_\rho \epsilon ^{abc}{\rho }_{\mu }^b{\rho }_{\nu }^c \end{aligned}$$

with the coupling constant given by \(g_\rho =\sqrt{2}m_\rho /f_\pi \) [41]. These tensors can be rearranged in the charge eigenstates so that the magnetic effect can be introduced directly by changing \(\partial _\mu \) to covariant derivative \(D_\mu \equiv \partial _\mu +i\,qA_\mu \) with q the particle charge. Then, we get the strength tensors of charge-definite \(\varvec{\rho }\) as

$$\begin{aligned} {\rho }_{\mu \nu }^0= & {} \partial _\mu {\rho }^0_\nu -\partial _\nu {\rho }^0_\mu +i\,g_\rho (\rho ^-_\mu \rho ^+_\nu -\rho ^-_\nu \rho ^+_\mu ), \end{aligned}$$
(3)
$$\begin{aligned} {\rho }_{\mu \nu }^\pm= & {} D_\mu ^\pm {\rho }^\pm _\nu -D_\nu ^\pm {\rho }^\pm _\mu ,\ D_\mu ^\pm \equiv \partial _\mu \pm ieA_\mu \mp i\,g_\rho {\rho }^0_\mu , \end{aligned}$$
(4)

where we find that \({\rho }_{\mu \nu }^\pm \) can be simply present in Abelian forms with the redefinition of the gauge field as \(A_\mu -{g_\rho \over e}{\rho }^0_\mu \). In accordance with the spin eigenstates, the corresponding covariant derivatives are related to the Lorentz components as:

$$\begin{aligned} D_0^{(\pm )}=D_z^{(\pm )},\ D_{\uparrow /\downarrow }^{(\pm )}=i{D_x^{(\pm )}\mp i\,D_y^{(\pm )}\over \sqrt{2}} \end{aligned}$$

for both neutral and charged \(\rho \) mesons. Considering a constant magnetic field along z direction, we choose the symmetric gauge for the vector potential: \(A_\mu =(0,By/2,-Bx/2,0)\). Then, as introduced in Ref. [42], the strength tensor couplings to the EM field in Eq. (2) become explicitly

$$\begin{aligned} \pm i{e\over 2}F^{\mu \nu }{\rho }_\mu ^\mp {\rho }_\nu ^\pm =\pm {1\over 2}eB\left( {\rho }_{\downarrow }^\mp {\rho }_\uparrow ^\pm -{\rho }_{\uparrow }^\mp {\rho }_\downarrow ^\pm \right) . \end{aligned}$$

Furthermore, according to the discussions in Refs. [43, 44], the effect of rotation along z direction can be simply introduced through the modification of temporal derivative \(\partial _t\) to

$$\begin{aligned} D_t=\partial _t-i\,\Omega \left( {\hat{L}}_z+{\hat{S}}_z\right) , \end{aligned}$$

where \({\hat{L}}_z\equiv -i(x\partial _y-y\partial _x)\) and \({\hat{S}}_z\) are the orbital angular momentum (OAM) and spin operators, respectively.

Now, without applying any boundary condition to a cylindrical system with radius R, the diagonal kinetic parts of the Lagrangian can be expressed explicitly on the basis of energy \(k_4\), momentum \(k_3\), Landau level n and OAM quantum number l as

$$\begin{aligned} \mathcal{L}_k= & {} -{1\over 2}{{\pi }^0_{-l}\left[ (k_4-i\,\Omega l)^2+{k}_l^2+{k}_3^2+m_\pi ^2\right] {\pi }^0_l}\nonumber \\&\quad -{1\over 2}{{\pi }^\pm _{n,\pm l}\left[ (k_4\pm i\,\Omega l)^2+(2n+1)|eB|+k_3^2+m_\pi ^2\right] {\pi }^\mp _{n,\mp l}}\nonumber \\&\quad -{1\over 2} {\rho }^{0}_{-s,-l}\left[ (k_4-i\,\Omega (l+s))^2+{{k}_l^2}+{k}_3^2+m_\rho ^2\right] {\rho }^{0}_{s,l}\nonumber \\&\quad +{1\over 2}{\rho }^{0}_{t,-l}\left[ (k_4-i\,\Omega (l+s))^2+{k}_l^2+{k}_3^2+m_\pi ^2\right] {\rho }^{0}_{t,l}\nonumber \\&\quad -{1\over 2} {\rho }^{\pm }_{-s,n,\pm l}\left[ (k_4-i\,\Omega (\mp l+s))^2+(2n+1\pm 2s)|eB|\right. \nonumber \\&\quad \left. +\,{k}_3^2+m_\rho ^2\right] {\rho }^{\mp }_{s,n,\mp l}\nonumber \\&\quad +\,{1\over 2} {\rho }^{\pm }_{t,n,\pm l}\left[ (k_4\pm i\,\Omega l)^2+(2n+1)|eB|+{k}_3^2+m_\rho ^2\right] {\rho }^{\mp }_{t,n,\mp l},\nonumber \\ \end{aligned}$$
(5)

where particularly the summations over nls should be understood with \(s=-1,0,1\), \(n\ge 0\), \(l\in (-\infty ,\infty )\) for neutral particles and \(l\in (-n,[{\mathcal {N}}]-n)\) for charged ones [43]. Note that the OAM is given by \(-l\) for negative charged particle and \([{\mathcal {N}}]\equiv \left[ {|qB| R^2\over 2}\right] \) is the number of magnetic flux quantization. Especially, we choose the simplest Lorentz gauge \(D_\mu \varvec{\rho }^\mu =0\) for \(\rho \) mesons, then the commutations \([D_\mu ,D_\nu ]\) from \(\varvec{\rho }_{\mu \nu }^\dagger \cdot \varvec{\rho }^{\mu \nu }\) give rise to extra kinetic terms the same as the strength tensor couplings. The left particle coupling parts of the Lagrangian involve the self-interactions of \(\rho \) mesons, which are quite the same as those of W/Z bosons in the electroweak theory, and the \(\rho \pi \pi \) interactions whose explicit forms can be illuminated as

$$\begin{aligned} \mathcal{L}_{\rho \pi \pi }= & {} g_\rho \left\{ \left[ \left( {\rho }^{-}_{\downarrow \uparrow ,n,-l}{\pi }^+_{n', l'}-{\rho }^{+}_{\downarrow \uparrow ,n,l}{\pi }^-_{n',-l'}\right) \left( \pm {k_{l''}''}{\pi }^0_{l''\mp 1}\right) /{\sqrt{2}}-\left( {\rho }^{-}_{0,n,-l}{\pi }^+_{n', l'}-{\rho }^{+}_{0,n,l}{\pi }^-_{n',-l'}\right) k_3''{\pi }^0_{l''}-i\left( {\rho }^{-}_{t,n,-l}{\pi }^+_{n', l'}\right. \right. \right. \nonumber \\&\left. \left. -{\rho }^{+}_{t,n,l}{\pi }^-_{n',-l'}\right) (k_4-i\,\Omega l''){\pi }^0_{l''}\right] -\left[ \left( {\rho }^{-}_{\downarrow ,n,-l}\sqrt{(n''+1)|eB|}{\pi }^+_{n''+1, l''-1} +{\rho }^{+}_{\downarrow ,n,l}\sqrt{n''|eB|}{\pi }^-_{n''- 1,-l''-1}\right) {\pi }^0_{l''- 1}\right. \nonumber \\&\quad -\left( {\rho }^{-}_{\uparrow ,n,-l}\sqrt{n''|eB|}{\pi }^+_{n''-1, l''+1}+{\rho }^{+}_{\uparrow ,n,l}\sqrt{(n''+1)|eB|}{\pi }^-_{n''+ 1,-l''+1}\right) {\pi }^0_{l''+1} -\left( {\rho }^{-}_{0,n,-l}k_3'{\pi }^+_{n', l'}\right. \left. -{\rho }^{+}_{0,n,l}k_3'{\pi }^-_{n',-l'}\right) {\pi }^0_{l''}\nonumber \\&\left. -i\left( {\rho }^{-}_{t,n,-l}(k_4-i\,\Omega l'){\pi }^+_{n', l'}-{\rho }^{+}_{t,n,l}(k_4+i\,\Omega l'){\pi }^-_{n',-l'}\right) {\pi }^0_{l''}\right] \nonumber \\&\quad +\left[ {\rho }^{0}_{\downarrow ,l}\left( {\pi }^-_{n',-l'}\sqrt{(n''\!+\!1)|eB|}{\pi }^+_{n''+1, l''-1}\right. \!+\!{\pi }^+_{n', l'}\sqrt{n''|eB|}{\pi }^-_{n''- 1,-l''-1}\right) \!-\!{\rho }^{0}_{\uparrow ,l} \!\times \! \left( {\pi }^-_{n',-l'}\sqrt{n''|eB|}{\pi }^+_{n''-1, l''+1} +{\pi }^+_{n', l'}\right. \nonumber \\&\quad \left. \times \sqrt{(n''+1)|eB|}{\pi }^-_{n''+ 1,-l''+1}\right) \left. \left. -{\rho }^{0}_{0,l}\left( {\pi }^-_{n',-l'}k_3''{\pi }^+_{n'', l''}-{\pi }^+_{n', l'}k_3''{\pi }^-_{n'',-l''}\right) \right. \right. \nonumber \\&\quad \left. \left. \quad -i{\rho }^{0}_{t,l}\left( {\pi }^-_{n',-l'}(k_4-i\,\Omega l''){\pi }^+_{n'', l''}\right. \right. \right. \left. \left. \left. -{\pi }^+_{n', l'}(k_4+i\,\Omega l''){\pi }^-_{n'',-l''}\right) \right] \right\} .\nonumber \\ \end{aligned}$$
(6)

Here, as before, the summations over the quantum numbers of all the relevant particles should be understood. We note that the coordinate integrations haven’t been carried out yet in Eq. (6), that is why there seem no connections among the quantum numbers of the interacting particles.

In the following, we skip the complicated interaction parts and only focus on the kinetic parts of the Lagrangian to get some physical intuitions. From Eq. (5), we surprisingly notice that rotation even induces effective chemical potentials for neutral pion and rho, thus the \(\pi ^0\ (\rho ^0)\) condensation is expected when \(|\Omega l|>m_{\pi }\ (|\Omega (l+s)|>m_{\rho })\). Moreover, in the presence of a magnetic field, the \(\pi ^0\) seems much easier to condense than \(\pi ^\pm \) with the condition for the latter: \(|\Omega l|>\sqrt{m_\pi ^2+|eB|}\). All these puzzles can be consistently solved when we combine the restriction of causality together with boundary conditions [43, 45, 46]. As a matter of fact, causality constrains the angular velocity to \(\Omega \le 1/R\) and the Dirichlet boundary conditions, requiring the wave functions to vanish at the boundary R, discretizes the transverse momentum such that \(|k_{l}|>(|l|+2)/R\) for each l. Thus, the excitation energy \(E_0=({k}_l^2+{k}_3^2+m^2)^{1/2}\) of the neutral particle satisfies

$$\begin{aligned} E_0>|k_{l}|>|\Omega (l+s)|, \end{aligned}$$

which eventually prevents any accumulation of \(\pi ^0\) or \(\rho ^0\) meson.

Next, we discuss a bit more about the effect of boundary condition on \(\pi ^\pm \) in a background magnetic field. For \(\pi ^+\) with \(l>0\), the excitation energy for transverse dynamics is [30]

$$\begin{aligned} E_{nl}(eB)\equiv \sqrt{m_\pi ^2+|eB|(2\lambda _l^n+1)} \end{aligned}$$

with the boundary condition

$$\begin{aligned} _1F_1(-\lambda _l^n,l+1,{\mathcal {N}})=0 \end{aligned}$$

and the quasi Landau levels \(0\le \lambda _l^0<\lambda _l^1<\lambda _l^2<\dots \). We’ve checked numerically that there is always a window of l satisfying \(l^2>2(2\lambda _l^0+1){\mathcal {N}}\) when \({\mathcal {N}}\gtrsim 7\), which means the unstable condition \(\Omega l>E_{0l}(eB)\) can be realized for large enough \(\Omega \) and eB. This is consistent with \(\pi ^\pm \) superfluid found in Ref. [30]. However, one problem is still left: if we don’t artificially set \(l\le [{\mathcal {N}}]\) as in Ref. [30], it seems that the lowest total particle energy \(E_{0l}^\Omega =E_{0l}(eB)-\Omega l\) is not bound from below, which would cause a disaster of infinite condensate density according to Ref. [30]. Actually, the answer is that \(\lambda _l^0\) becomes quite large for large l, which then makes sure that \(E_{0l}^\Omega >-\infty \) in the limit \(l\rightarrow \infty \).

For the purpose of intuition, we show the scaled dimensionless energy

$$\begin{aligned} {\tilde{E}}_{0l}^\Omega \equiv {\sqrt{|eB|(2\lambda _l^0+1)}-{l\over R}\over \sqrt{|eB|}}=\sqrt{2\lambda _l^0+1}-{l\over \sqrt{2{\mathcal {N}}}} \end{aligned}$$

for different values of \({\mathcal {N}}\) in Fig. 1, where positive features can always be identified at large l. And with the increasing of \({\mathcal {N}}\), that is, the enhancement of eB for a given R, more \(\pi ^+\) can be condensed as more are trapped in the system. It should be pointed out that finite lower boundaries exist for the total energies of any charged particles.

Fig. 1
figure1

The dimensionless energy \({\tilde{E}}_{0l}^\Omega \) as a function of the orbital angular momentum l for different values of \({\mathcal {N}}\)

In pure magnetic field, it was found that the degeneracy of l is automatically restricted to \(\le [{\mathcal {N}}]\) for the lowest Landau level when the boundary condition is applied [43]. We even check in advance that the degeneracy decreases with the Landau level n, see the plains in Fig. 2. Nevertheless, for the case \({\mathcal {N}}=15\) in Fig. 1, the much wider unstable window of l disfavors the use of the artificial upper bound \([{\mathcal {N}}]\) for l when large angular velocity (\(\Omega \lesssim 1/R\)) is involved.

Fig. 2
figure2

The three lowest quasi Landau levels \(\lambda _l^n\ (n=0,1,2)\) as functions of the orbital angular momentum l for \({\mathcal {N}}=100\)

Finally, turn to the charged \(\rho \) vector mesons, the story is quite different because of their non-vanishing spins. In the presence of \(\mathbf{B}\parallel \varvec{\Omega }\), the effective mass of \(\rho ^+_{\uparrow }\) or \(\rho ^-_\downarrow \) decreases as \(\sqrt{m_\rho ^2+|eB|(2\lambda _l^0-1)}\) on one hand [24], the effective isospin chemical potential increases as \(\Omega (l+1)\) on the other hand. Then, it seems that \(\rho ^+_{\uparrow }\) condensation would overwhelm the \(\pi ^+\) condensation to be the true ground state when \(\Omega \) is large enough that

$$\begin{aligned} \Omega (l+1)-\sqrt{m_\rho ^2+|eB|(2\lambda _l^0-1)}>\Omega l-E_{0l}(eB)>0. \end{aligned}$$

As the VW theorem might forbid the decreasing of composite \(\rho ^+_{\uparrow }\) mass to zero in pure magnetic field [33,34,35,36], the estimation of the \(\rho ^+_{\uparrow }\) mass is not correct at all for large B in the point particle picture. However, as mentioned in the introduction, \(\Omega \) invalids the proof of the theorem thus the isospin chemical potential effect of \(\Omega (l+1)\) can still be qualitatively correct in the point particle picture.

Nambu–Jona-Lasinio model in rotating frame

In order to explore the possibility of charged rho condensation more realistically, we adopt the SU(3) NJL model with ud and s quarks the fundamental degrees of freedom [47]. In the rotating frame, the action of the system can be conveniently given in curved spacetime by

$$\begin{aligned} \mathcal{S}=\int d^4x \sqrt{-\det (g_{\mu \nu })}\mathcal{L}(\bar{\psi },\psi ), \end{aligned}$$
(7)

where the Lagrangian density can be extended from the usual one [47, 48] to

(8)

by further adopting the four fermion vector interaction channels with coupling constant \(G_V\). Compared to the two-flavor NJL model, the advantage of three-flavor NJL model is that: there the vacuum superconductivity or \(\rho ^\pm \) superconductor cannot happen due to the mass splitting of quarks in pure magnetic field [35], which is consistent with lattice QCD simulations [33, 34, 36].

In the Lagrangian, \(\psi =(u,d,s)^T\) represents the three-flavor quark field and \(m_0=\mathrm{diag}(m_{\mathrm{0u}},m_{\mathrm{0d}},m_{\mathrm{0s}})\) is the current quark mass matrix. The longitudinal and transverse covariant derivatives with \(\mathbf{B}\parallel \varvec{\Omega }\) effect are defined, for symmetric gauge, respectively as

$$\begin{aligned} D_0=\partial _t-i\Omega \left( {\hat{L}}_z+{\hat{S}}_z\right) ,~D_3=\partial _z \end{aligned}$$

and

$$\begin{aligned} D_1=\partial _x+iQ\,By/2,~D_2=\partial _y-iQ\,Bx/2 \end{aligned}$$

with the charge matrix \(Q=\mathrm{diag}(q_{\mathrm{u}},q_{\mathrm{d}},q_\mathrm{s})\). For the four-fermion interaction terms, \(\lambda ^0=\sqrt{2\over 3}I\) and Gell-Mann matrices \(\lambda ^i~(i=1,\dots ,8)\) are defined in three-flavor space, so the extra diagonal terms \(({\bar{\psi }}\lambda ^{3}\psi )^2\) and \(({\bar{\psi }}\lambda ^{8}\psi )^2\) allow mass splitting among all the flavors in contrary to the two-flavor case [35]. The \(U_A(1)\) symmetry violating term \(\mathcal{L}_6\) [49] only involves scalar-pseudoscalar channels with the determinant defined in flavor space, \(\Gamma ^\pm =1\pm \gamma _5\) and K the coupling constant. Now, we only consider nonzero chiral condensations \(\sigma _\mathrm{i}\equiv \langle \bar{\psi }^i{\psi }^i\rangle \), where the correspondence between the Arabian denotations \(i=1,2,3\) and the more explicit Latin ones \(\mathrm{f=u,d,s}\) should be understood for the flavors. The six fermion interactions in \(\mathcal{L}_6\) can be reduced to effective four fermion ones in Hartree approximation [47], then the Lagrangian density only involves four fermion effective interactions:

(9)

where the non-vanishing elements of the symmetric coupling matrices \(G^\pm \) are given by [47]

$$\begin{aligned}&G_{00}^\mp =G_S\mp {K\over 3}\sum _{\mathrm{f=u,d,s}}\sigma _\mathrm{f},~G_{11}^\mp =G_{22}^\mp =G_{33}^\mp =G_S\pm {K\over 2}\sigma _s,\nonumber \\&G_{44}^\mp =G_{55}^\mp =G_S\pm {K\over 2}\sigma _\mathrm{d},~G_{66}^\mp =G_{77}^\mp =G_S\pm {K\over 2}\sigma _{\mathrm{u}},\nonumber \\&G_{88}^\mp =G_S\mp {K\over 6}(\sigma _s-2\sigma _{\mathrm{u}}-2\sigma _\mathrm{d}),~G_{08}^\mp =\mp {\sqrt{2}K\over 12}(2\sigma _s\!-\!\sigma _\mathrm{u}\!-\!\sigma _{\mathrm{d}}),\nonumber \\&\quad ~G_{38}^\mp =-\sqrt{2}G_{03}^\mp =\mp {\sqrt{3}K\over 6}(\sigma _{\mathrm{u}}\!-\!\sigma _{\mathrm{d}}). \end{aligned}$$
(10)

In the case \(\langle \sigma _i\rangle \ne 0\), the inverse quark propagators of different flavors are given by the introductions of the dynamical masses and covariant derivatives as

(11)

By using the eigenfunction reconstruction method, we have given the propagator of a fermion with positive or negative charge [37]; so the u and d/s quark propagators are respectively

$$\begin{aligned} \!\!\!S_\mathrm{u}(x,x')= & {} \sum _{n=0}^\infty \sum _l\int \int {dp_0dp_z\over (2\pi )^2}{i~e^{-ip_0(t-t^\prime )+ip_z(z-z^\prime )}\over \left( {p}_0^{l+}\right) ^2-(\varepsilon _n^u)^2+i\epsilon }\nonumber \\&\times \Bigg \{\left[ \mathcal{P}_\uparrow \chi _{n,l}^+(\theta ,r)\chi _{n,l}^{+*}(\theta ',r')+\mathcal{P}_\downarrow \chi _{n-1,l+1}^+(\theta ,r)\chi _{n-1,l+1}^{+*}(\theta ',r')\right] \left( \gamma ^0{p}_0^{l+}-\gamma ^3p_z+m_u\right) \nonumber \\&-\left[ \mathcal{P}_\uparrow \chi _{n,l}^+(\theta ,r)\chi _{n-1,l+1}^{+*}(\theta ',r')+\mathcal{P}_\downarrow \chi _{n-1,l+1}^+(\theta ,r)\chi _{n,l}^{+*}(\theta ',r')\right] \sqrt{2n |qB|}\gamma ^2\Bigg \}_{q\rightarrow q_{\mathrm{u}}}, \end{aligned}$$
(12)
$$\begin{aligned} S_\mathrm{d/s}(x,x')= & {} \sum _{n=0}^\infty \sum _l\int _{-\infty }^{\infty }{dp_0dp_z\over (2\pi )^2}{i~e^{-ip_0(t-t^\prime )+ip_z(z-z^\prime )}\over \left( {p}_0^{l-}\right) ^2-(\varepsilon _n^{d/s})^2+i\epsilon }\nonumber \\&\quad \times \Bigg \{\left[ \mathcal{P}_\uparrow \chi _{n-1,l-1}^{-}(\theta ,r)\chi _{n-1,l-1}^{-*}(\theta ',r') +\mathcal{P}_\downarrow \chi _{n,l}^{-}(\theta ,r)\chi _{n,l}^{-*}(\theta ',r')\right] \left( \gamma ^0{p}_0^{l-}-\gamma ^3p_z+m_\mathrm{d/s}\right) \nonumber \\&\quad +\left[ \mathcal{P}_\uparrow \chi _{n-1,l-1}^{-}(\theta ,r)\chi _{n,l}^{-*}(\theta ',r') +\mathcal{P}_\downarrow \chi _{n,l}^{-}(\theta ,r)\chi _{n-1,l-1}^{-*}(\theta ',r')\right] \sqrt{2n |qB|}\gamma ^2\Bigg \}_{q\rightarrow q_{\mathrm{d}}}, \end{aligned}$$
(13)

where \({p}_0^{ls}=p_0+\Omega \left( l+s{1\over 2}\right) \), the dispersion relations \(\varepsilon _n^i=(p_z^2+2n|q_iB|+m_i^2)^{1/2}\) and \(\mathcal{P}_{\uparrow /\downarrow }={1\over 2}(1\pm \sigma ^{12})\) are the spin projectors. Here, the normalized auxiliary functions are defined for positive and negative charged particles respectively as

$$\begin{aligned}&\chi _{n,l}^+(\theta ,r)=\left[ {|qB|\over 2\pi }{ n!\over (n\!+\!l)!}\right] ^{1\over 2}{e^{i\, l\theta }}~{\tilde{r}}^le^{-{\tilde{r}}^2/2}L_n^l\left( {\tilde{r}}^2\right) , \end{aligned}$$
(14)
$$\begin{aligned}&\chi _{n,l}^{-}(\theta ,r)=\left[ {|qB|\over 2\pi }{ n!\over (n\!-\!l)!}\right] ^{1\over 2}{e^{i\, l\theta }}~{\tilde{r}}^{-l}e^{-{\tilde{r}}^2/2}L_n^{-l}\left( {\tilde{r}}^2\right) , \end{aligned}$$
(15)

where the dimensionless radius \({\tilde{r}}^2=|qB|r^2/2\) and the Laguerre polynomial \(L_n^l(x)\) is nonvanishing only for \(n\ge 0\). Actually, in a rotating system, a boundary must be applied due to causality, then the propagators would no longer keeps the forms of Eqs. (12) and (13). But for convenience, we still adopt these forms and constrain the OAM as \(l\in \left[ -n,{\mathcal {N}}-n\right] \) [38]. Armed with that, the quark masses can be evaluated through the gap equations given by the self-consistent definitions of chiral condensations as:

$$\begin{aligned} \sigma _i\equiv \langle \bar{\psi }^i{\psi }^i\rangle =-{i\over V_4}\mathrm{Tr}~S_{i}. \end{aligned}$$
(16)

By adopting vacuum regularization, the explicit form of the gap equations are

$$\begin{aligned} -\sigma _{\mathrm{f}}= & {} N_c{{m_\mathrm{f}}^3\over 2\pi ^2}\Big [\tilde{\Lambda }_\mathrm{f}\Big ({1+\tilde{\Lambda }_\mathrm{f}^2}\Big )^{1\over 2}-\ln \Big ({{\tilde{\Lambda }}_{\mathrm{f}}} +\Big ({1+\tilde{\Lambda }_\mathrm{f}^2}\Big )^{1\over 2}\Big )\Big ]\nonumber \\&+N_c{m_\mathrm{f}\over 4\pi ^2}\int _0^\infty {ds\over s^2}e^{-{m_\mathrm{f}}^2s}\left( {q_{\mathrm{f}}Bs \over \tanh (q_{\mathrm{f}}Bs)}-1\right) \nonumber \\&-N_cm_{\mathrm{f}}\sum _{n=0}^{n_{\mathrm{max}}}{1\over S}\sum _{l=0}^{{\mathcal {N}}^{\mathrm{f}}}\int _{-\infty }^{\infty }{dp_z\over \pi }{\alpha _n\over \varepsilon _n^{\mathrm{f}}} \Big [f(\varepsilon _n^{\mathrm{f}}+\Omega _{nl})+f(\varepsilon _n^{\mathrm{f}}-\Omega _{nl})\Big ]\nonumber \\ \end{aligned}$$
(17)

with the reduced cutoff \(\tilde{\Lambda }_{\mathrm{f}}={\Lambda /m_\mathrm{f}}\). Compared to that given in Ref. [37] but implicitly implied, the Landau levels are cut off by \(n_\mathrm{max}~(\ll N_{\mathrm{f}})\) here, which was checked to be a good approximation for large B and \(\Omega =0\).

For a continuous transition, the effective potential can be expressed as the form in Ginzburg-Landau (GL) theory

$$\begin{aligned} V_{\mathrm{eff}}(\sigma _{\mathrm{f}},\Delta )=V_{\mathrm{eff}}(\sigma _\mathrm{f},0)+\mathcal{A}~\Delta ^2+\mathcal{B}~\Delta ^4+\dots , \end{aligned}$$
(18)

where \(V_{\mathrm{eff}}(\sigma _{\mathrm{f}},0)\) is the corresponding thermodynamic potential giving rise to the gap equations in Eq. (17). We note that \(\Delta \) can be an order parameter for any kind of mesonic superfluid or superconductor with the relevant coefficients \(\mathcal{A}\) and \(\mathcal{B}\) determined by their interactions with quarks. To avoid too much complexity, we assume the transition is solely determined by the quadratic one \(\mathcal{A}\) [37]: If \(\mathcal{A}<0\), the meson condensation is favored; and if \(\mathcal{A}_a<\mathcal{A}_b<0\), we would assume meson a is more preferred to condensate than meson b. We’ve discovered previously that \(\mathcal{A}\) is almost consistent with the inverse mesonic propagator in random phase approximation (RPA) except for some subtle discussions on the Schwinger phases of charged mesons [37, 38, 50]. As illuminated in Ref. [35], the bare form of the coefficient is given by

$$\begin{aligned} \mathcal{A}={1\over 4G}+\Pi \end{aligned}$$

with the polarization function defined through the fermion loop as

$$\begin{aligned} \Pi ={i\over V_4}\mathrm{Tr}\left[ S(x,y)\Gamma _{M*}S(y,x)\Gamma _{M}e^{-i\Phi _M}\right] . \end{aligned}$$
(19)

Here, \(V_4\) is the space-time volume, the trace should be taken over the internal and coordinate spaces, and \(e^{-i\Phi _M}\) is the compensated Schwinger phase.

Calculations of the quadratic coefficient

This section is mainly devoted to calculating the quadratic efficient explicitly. The interaction vertices between quarks and (pseudo-)scalar and vector mesons have been listed in Ref. [35] as:

$$\begin{aligned}&\Gamma _{\sigma /\sigma ^*}=-1,~\Gamma _{\pi ^0/{\pi ^0}^*}=-i\gamma ^5\tau _3,~\Gamma _{\pi _\pm }=-i\gamma ^5\tau _\pm ,~\Gamma _{\bar{\omega }_\mu /\bar{\omega }_\mu ^*}=\bar{\gamma }_\mu ^\pm ,\nonumber \\&\quad ~\Gamma _{\bar{\rho }_{0\mu }/\bar{\rho }_{0\mu }^*} =\bar{\gamma }_\mu ^\pm \tau _3,~\Gamma _{\bar{\rho }_{\pm \mu }}=\bar{\gamma }_\mu ^\pm \tau _\pm , \end{aligned}$$
(20)

where \(\bar{\gamma }^{\pm }_\mu =(\gamma _0,{\gamma _1\pm i\gamma _2\over \sqrt{2}},{\gamma _1\mp i\gamma _2\over \sqrt{2}},\gamma _3)\). In the following, we mainly focus on the \(\bar{\rho }^+_1\) mode, that is, the rho meson with spin long the magnetic field. The insertion of the fermion propagators from Eqs. (12) and (13) into the polarization function Eq. (19) is explicitly

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}={-i\over S}\sum _{n=0}^{n_\mathrm{max}}\sum _l\sum _{n'=0}^{n_\mathrm{max}}\sum _{l'}\int _{-\infty }^{\infty }{dp_0\over 2\pi }\int _{-\infty }^{\infty }{dp_z\over 2\pi } ~\mathrm{Tr}\Bigg \{\left[ \mathcal{P}_\uparrow \chi _{n,l}^+(\theta ,r)\chi _{n,l}^{+*}(\theta ',r') +\mathcal{P}_\downarrow \chi _{n-1,l+1}^{+}(\theta ,r)\chi _{n-1,l+1}^{+*}(\theta ',r')\right] \nonumber \\&\quad \times \left( \gamma ^0{p}_0^{l+}-\gamma ^3p_z+m_u\right) -\left[ \mathcal{P}_\uparrow \chi _{n,l}^{+}(\theta ,r)\chi _{n-1,l+1}^{+*}(\theta ',r')+\mathcal{P}_\downarrow \chi _{n-1,l+1}^{+}(\theta ,r)\chi _{n,l}^{+*}(\theta ',r')\right] \gamma ^2\sqrt{2n q_uB}\Bigg \}\nonumber \\&\quad \times \Bigg \{-\left[ \mathcal{P}_\downarrow \chi _{n'-1,l'-1}^{-}(\theta ',r')\chi _{n'-1,l'-1}^{-*}(\theta ,r)+\mathcal{P}_\uparrow \chi _{n',l'}^{-}(\theta ',r')\chi _{n',l'}^{-*}(\theta ,r)\right] \left( \gamma ^0{p}_0^{l'-}{-}\gamma ^3p_z{-}m_d\right) {\gamma ^1{+}i\gamma ^2\over \sqrt{2}}\nonumber \\&\quad -\left[ \mathcal{P}_\downarrow \chi _{n'-1,l'-1}^{-}(\theta ',r')\chi _{n',l'}^{-*}(\theta ,r) +\mathcal{P}_\uparrow \chi _{n',l'}^{-}(\theta ',r')\chi _{n'-1,l'-1}^{-*}(\theta ,r)\right] \nonumber \\&\quad \times \gamma ^2\sqrt{2n'|q_dB|}{\gamma ^1-i\gamma ^2\over \sqrt{2}}\Bigg \}{\gamma ^1-i\gamma ^2\over \sqrt{2}}{e^{-i\Phi }\over \left[ \left( {p}_0^{l+}\right) ^2-(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{l'-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }, \end{aligned}$$
(21)

where the trace is over the Dirac and the coordinate spaces. By completing the trace over the Dirac space, the expression becomes quite simple:

$$\begin{aligned} \Pi _{\bar{\rho }^+_1}= & {} {-4N_ci\over S}\sum _{n=0}^{n_\mathrm{max}}\sum _l\sum _{n'=0}^{n_\mathrm{max}}\sum _{l'}\sum _{r,r'}\sum _{\theta ,\theta '}\int _{-\infty }^{\infty }{dp_0\over 2\pi }\int _{-\infty }^{\infty }{dp_z\over 2\pi } {e^{-i\Phi }\over \left[ \left( {p}_0^{l+}\right) ^2 -(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{l'-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }\nonumber \\&\times \left( {p}_0^{l+}{p}_0^{l'-}-p_z^2-m_um_d\right) \chi _{n,l}^{+}(\theta ,r)\chi _{n,l}^{+*}(\theta ',r')\chi _{n',l'}^{-}(\theta ',r')\chi _{n',l'}^{-*}(\theta ,r), \end{aligned}$$
(22)

where we define \(\sum _{r,r'}=\int _0^\infty rdr\int _0^\infty r'dr'\) and \(\sum _{\theta ,\theta '}=\int _0^{2\pi }d\theta \int _0^{2\pi }d\theta '\). Consistent with the form in pure magnetic field [35] but different from that of charged pion [37], only the term with numerator independent of Landau levels survives and there is only one kind of combination of \(\chi ^{+}\chi ^{+*}\) and \(\chi ^{-}\chi ^{-*}\). By the way, for the corresponding axial vector \({\bar{a}}^+_1\) with interaction indices \(\Gamma _{{\bar{a}}^+_1}=i\gamma ^5\Gamma _{\bar{\rho }_1^+}\), the polarization function is the same as that of \(\bar{\rho }^+_1\) except that the sign of the mass term is changed, that is, \(-m_um_d\rightarrow +m_um_d\). We’ve shown in Ref. [35] that the contribution of the mass term is negative to \(\Pi _{\bar{\rho }^+_1}\), hence \(m_{{\bar{a}}^+_1}>m_{\bar{\rho }^+_1}\) in the chiral symmetry breaking phase. Then it turns out that the \({\bar{a}}^+_1\) superconductor is neither favored in magnetic field, but it still needs to be checked in \(\mathbf{B}\parallel \varvec{\Omega }\) where this term can be positive for \(\bar{\rho }^+_1\).

For Schwinger phase in Minkowski space

To calculate Eq. (22) further, we choose the Schwinger phase of the form in Minkowski space, that is, \(\Phi _M=e\int _x^y{A}_\mu (z) d{z}_\mu ={eB\over 2}\sin (\theta -\theta ')rr'\). Then, the integrals over the polar angles can be completed to give

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}={-16N_ci\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d}\sum _{r,r'} \int _{-\infty }^{\infty }{dp_0\over 2\pi }\int _{-\infty }^{\infty }{dp_z\over 2\pi } {e^{-{eB\over 4}(r^2+{r'}^2)}\left( {p}_0^{(l-n)+}{p}_0^{(n'-l')-}-p_z^2-m_um_d\right) \over \left[ \left( {p}_0^{(l-n)+}\right) ^2-(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }{n!n'!\over l!l'!}\nonumber \\&\quad \times \left( {q_uB\over 2}\right) ^{l-n+1}\left( {|q_dB|\over 2}\right) ^{l'-n'+1}J_{l+l'-n-n'}\left( {eB\over 2}rr'\right) (rr')^{l+l'-n-n'}{F}_{nl,n'l'}(q_uB,|q_dB|;r,r'), \end{aligned}$$
(23)

where the auxiliary function F is defined as

$$\begin{aligned}&F_{nl,n'l'}(q_uB,|q_dB|;r,r')\nonumber \\&\quad \equiv \prod _{x=r,r'}L_n^{l-n}\left( {q_uB ~x^2\over 2}\right) L_{n'}^{l'-n'}\left( {|q_dB| ~x^2\over 2}\right) . \end{aligned}$$
(24)

Here, we find that the LLL combination of u and d quarks contribute to the term \({F}_{nl,n'l'}(q_uB,|q_dB|;r,r')\) with \(n=n'=0\), due to the special structure of \(\chi ^{+}\chi ^{+*}\) and \(\chi ^{-}\chi ^{-*}\) in Eq. (22). For charged pion, this kind of combination is absent [37] due to the fact that the LLLs of of u and d quarks cannot form spin singlet at all.

For convenience, we redefine the radii to dimensionless ones \({\bar{r}}=(eB/2)^{1/2} r\) and \({\bar{r}}'=(eB/2)^{1/2} r'\), then Eq. (23) becomes

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}={-16N_ci\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d} \int _{-\infty }^{\infty }\!{dp_0\over 2\pi }\nonumber \\&\quad \int _{-\infty }^{\infty }\!{dp_z\over 2\pi } {\left( {p}_0^{(l-n)+}{p}_0^{(n'-l')-}\!\!-\!p_z^2\!-\!m_um_d\right) \! \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)\over \left[ \left( {p}_0^{(l-n)+}\right) ^2-(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }, \end{aligned}$$
(25)
$$\begin{aligned}&\!\! \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)={n!n'!\over l!l'!}{\tilde{q}}_u^{l-n+1}{|{\tilde{q}}_d|}^{l'-n'+1}\nonumber \\&\quad \sum _{{\bar{r}},{\bar{r}}'}e^{-{{\bar{r}}^2+({\bar{r}}')^2\over 2}}J_{l+l'-n-n'}\left( {\bar{r}}{\bar{r}}'\right) ({\bar{r}}{\bar{r}}')^{l+l'-n-n'}{F}_{nl,n'l'}(2{\tilde{q}}_u,2|{\tilde{q}}_d|;{\bar{r}},{\bar{r}}')\nonumber \\ \end{aligned}$$
(26)

with \({\tilde{q}}=q/e\). It is useful to transform the numerator \({p}_0^{(l-n)+}{p}_0^{(n'-l')-}-p_z^2-m_um_d\) of the integrand in Eq. (2526) to the following form:

$$\begin{aligned}&{1\over 2}\Bigg [\left( {p}_0^{(l-n)+}\right) ^2-(\varepsilon _n^u)^2+\left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2 \nonumber \\&\quad -\Omega _{nl,n'l'}^2+(m_u-m_d)^2+2n\,q_uB+2n'|q_dB|\Bigg ], \end{aligned}$$
(27)

where \(\Omega _{nl,n'l'}=(l+l'-n-n'+1)\Omega \). Then the polarization function becomes

$$\begin{aligned} \Pi _{\bar{\rho }^+_1}= & {} {-8N_ci\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d} \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)\int _{-\infty }^{\infty }\!{dp_0\over 2\pi }\int _{-\infty }^{\infty }\!{dp_z\over 2\pi }\nonumber \\&\times \left\{ {1\over \left( {p}_0^{(l-n)+}\right) ^2-(\varepsilon _n^u)^2}+{1\over \left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2}\right. \nonumber \\&\left. +{-\Omega _{nl,n'l'}^2+(m_u-m_d)^2+2n\,q_uB+2n'|q_dB|\over \left[ \left( {p}_0^{(l-n)+}\right) ^2-(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }\right\} . \end{aligned}$$
(28)

Shifting to Euclidean space through the transformations: \(p_0\rightarrow i\omega _m\) and \(-i\int _{-\infty }^{\infty }\!{dp_0\over 2\pi }\rightarrow T\sum _{m=-\infty }^\infty \) and completing the summation over the fermion Matsubara frequency \(\omega _m=(2m+1)\pi T\), we have

$$\begin{aligned} \Pi _{\bar{\rho }^+_1}= & {} {-2N_c\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d} \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)\nonumber \\&\quad \sum _{s=\pm }\int _{-\infty }^{\infty }{dp_z\over (2\pi )}\Bigg \{\tanh \left( {\varepsilon _n^u-s~\Omega _{nl,{1\over 2}0}\over 2T}\right) {1\over \varepsilon _n^u}\Bigg [ 1\nonumber \\&+\left. {-\Omega _{nl,n'l'}^2+(m_u-m_d)^2+2n\,q_uB+2n'|q_dB|\over \left( \varepsilon _n^u-s~ \Omega _{nl,n'l'}\right) ^2-(\varepsilon _{n'}^d)^2}\Bigg ]\right. \nonumber \\&+\left( \varepsilon _{n'}^d\leftrightarrow \varepsilon _{n}^u,nl\leftrightarrow n'l',q_u\leftrightarrow |q_d|\right) \Bigg \}. \end{aligned}$$
(29)

The temperature and rotation dependent part can be separated out as \(\Pi _{\bar{\rho }^+_1}-\Pi _{\bar{\rho }^+_1}\big |_{\Omega \rightarrow 0, T\rightarrow 0},\) which should be convergent similar to that of charged pion [37]. Here, the subtracting term is just the polarization function in pure magnetic field, which has been regularized in Ref. [35] as \(\left[ \Pi _{\bar{\rho }^+_1}^B-\Pi _{\bar{\rho }^+_1}^{o(B^2)}\right] +\Pi _{\bar{\rho }^+_1}^\Lambda \). We close this section by listing the relevant terms:

$$\begin{aligned} \Pi _{\bar{\rho }^+_1}^B= & {} -{N_c\over 8\pi ^2}\!\!\int \!{\mathrm{d}s\over s}\!\!\int _{-1}^1\!\! {\mathrm{d}u}~{e^{-s\left[ m_{\mathrm{u}}^2u^+\!+m_\mathrm{d}^2u^-\right] }}\!\!\left( m_{\mathrm{u}}m_{\mathrm{d}}\!+\!{1\over s}\right) \!\!\nonumber \\&\quad \times \left[ 1\!+\!\tanh \left( q_\mathrm{u}Bsu^+\right) \right] \left[ 1\!-\!\tanh \left( q_\mathrm{d}Bsu^-\right) \right] \nonumber \\&\quad 1\over {\tanh \left( q_{\mathrm{u}}Bsu^+\right) \over q_{\mathrm{u}}Bs}+{\tanh \left( q_{\mathrm{d}}Bsu^-\right) \over q_{\mathrm{d}}Bs} \end{aligned}$$
(30)

with \(u^\pm =(1\pm u)/2\), \(\Pi _{\bar{\rho }^+_1}^{o(B^2)}\) is the weak B expansion of \(\Pi _{\bar{\rho }^+_1}^B\) to order \(o(B^2)\) and the term with three-momentum cutoff \(\Lambda \) is

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}^\Lambda =-N_c\int _0^\Lambda \!\! {k^2dk\over \pi ^2}\frac{(E_{\mathrm{u}}E_{\mathrm{d}}\!+\!{m_{\mathrm{u}}}{m_\mathrm{d}}\!+\!{1\over 3}k^2)}{E_{\mathrm{u}}E_{\mathrm{d}}(E_{\mathrm{u}}\!+\!E_\mathrm{d})}\nonumber \\&\quad -{N_c}\int _0^\Lambda {k^2dk\over 2\pi ^2}\left\{ {{q_\mathrm{u}B}\over (E_{\mathrm{u}}\!+\!E_{\mathrm{d}})^2}\left[ \left( \frac{E_\mathrm{u}E_{\mathrm{d}}\!+\!{m_{\mathrm{u}}}{m_{\mathrm{d}}}\!+\!{1\over 3}k^2}{E_\mathrm{u}^3}\!+\!{1\over E_{\mathrm{u}}}\!+\!{1\over E_\mathrm{d}}\right) \right. \right. \nonumber \\&\quad \left. \left. -\frac{(m_{\mathrm{u}}\!-\!m_\mathrm{d})^2\!+\!{4\over 3}k^2}{E_{\mathrm{u}}^2E_\mathrm{d}}\right] \!-\!(u\leftrightarrow d)\right\} . \end{aligned}$$
(31)

For Schwinger phase in curved space

Next, we choose the Schwinger phase of the form in curved space, that is, \(\Phi _M={eB\over 2}\sin [\theta -\theta '+\Omega (t-t')]rr'\). By taking variable transformation of the angle: \(\theta -\theta '\rightarrow \theta -\theta '-\Omega (t-t')\), we find that the corresponding polarization function can be modified from Eq. (2526) by changing \({p}_0^{(l-n)+}\) to \({p}_0^{(n'-l')+}\), that is,

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}={-16N_ci\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d} \int _{-\infty }^{\infty }\!{dp_0\over 2\pi }\int _{-\infty }^{\infty }\!{dp_z\over 2\pi }\nonumber \\&\quad \times {\left( {p}_0^{(n'-l')+}{p}_0^{(n'-l')-}\!\!-\!p_z^2\!-\!m_um_d\right) \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)\over \left[ \left( {p}_0^{(n'-l')+}\right) ^2-(\varepsilon _n^u)^2\right] \left[ \left( {p}_0^{(n'-l')-}\right) ^2-(\varepsilon _{n'}^d)^2\right] }.\nonumber \\ \end{aligned}$$
(32)

Then, in a similar process as the previous section, the summation over the Fermion Matsubara frequency gives

$$\begin{aligned}&\Pi _{\bar{\rho }^+_1}={-2N_c\over S}\sum _{n,n'=0}^{n_\mathrm{max}}\sum _{l=0}^{{\mathcal {N}}_u}\sum _{l'=0}^{{\mathcal {N}}_d} \mathcal{F}_{nl,n'l'}({\tilde{q}}_u,|{\tilde{q}}_d|)\sum _{s=\pm } \int _{-\infty }^{\infty }{dp_z\over (2\pi )}\nonumber \\&\quad \times \left\{ \tanh \left( {\varepsilon _n^u\!+\!s~\Omega _{{3\over 2}0,n'l'}\over 2T}\right) {1\over \varepsilon _n^u}+\tanh \left( {\varepsilon _{n'}^d-s~\Omega _{{1\over 2}0,n'l'}\over 2T}\right) {1\over \varepsilon _{n'}^d}\right. \nonumber \\&+\left[ {-\Omega ^2\!+\!(m_u\!-\!m_d)^2\!+\!2n\,q_uB\!+\!2n'|q_dB|}\right] \nonumber \\&\quad \left. \left[ {1\over \varepsilon _n^u}{\tanh \left( {\varepsilon _n^u\!+\!s~\Omega _{{3\over 2}0,n'l'}\over 2T}\right) \over \left( \varepsilon _n^u-s\,\Omega \right) ^2-(\varepsilon _{n'}^d)^2}+{1\over \varepsilon _{n'}^d}{\tanh \left( {\varepsilon _{n'}^d-s~\Omega _{{1\over 2}0,n'l'}\over 2T}\right) \over \left( \varepsilon _{n'}^d-s\,\Omega \right) ^2-(\varepsilon _n^u)^2}\right] \right\} . \end{aligned}$$
(33)

In contrary to that of charged pion [38], the angular velocity \(\Omega \) can still plays a role of effective isospin chemical potential to \(\bar{\rho }^+_1\) in this case, see the denominators. Finally, one should keep in mind that the regularization to Eq. (32) is performed in the same way as that of SP in Minkowski space.

Possibility of charged rho superconductor

In order to carry out numerical calculations, we choose the following parameters for the scalar-pseudoscalar sector: \(m_\mathrm{u}=m_{\mathrm{d}}=5.5~\mathrm{MeV}, m_{\mathrm{s}}=140.7~\mathrm{MeV}, \Lambda =602.3~\mathrm{MeV}, G_S\Lambda ^2=1.835\) and \(K\Lambda ^5=12.36\) [51]. To avoid artifacts, the vector coupling constant is fixed to \(G_V\Lambda ^2=2.527\) by fitting to the vacuum mass of \(\rho \) meson: \(m_\rho ^v=0.7~\mathrm{GeV}\) [35]. Following the study of Ref. [35], we consider a cylindrical system with the radius \(R=20/\sqrt{eB}\) and constrain the rotation by \(\Omega R\le 1\) for causality. As the upper limit of orbital angular momentum is limited by \(\mathcal{N}\), the B dependence of R cancels the B dependence of the upper limit and gives a natural number. Actually, what we are more interested in is the effect induced by changing the angular velocity rather than magnetic field, so this choice of R is fine for that purpose. As the original NJL model is not capable of explaining the inverse magnetic catalysis effect at finite temperature [19], we stick to the zero temperature case in the following numerical calculations.

Fig. 3
figure3

The evolutions of the dynamical quark masses \(m_{\mathrm{f}}\) (upper panel) and the quadratic GL expansion coefficients \(\mathcal{A}\) (lower panel) with the angular velocity \(\Omega \) at the magnetic field \(eB=0.5~\mathrm{GeV}^2\). In the lower panel, the coefficients of charged rho condensation are compared to those of charged pion for both choices of SP in Minkowski space and SP in curved space, denoted by “M” and “C”, respectively

We choose two strong enough magnetic fields for illumination: \(eB=0.5~\mathrm{GeV}^2\) and \(eB=1.5~\mathrm{GeV}^2\), which are on different sides of the minimum point of the \(\bar{\rho }^+_1\) mass found in our previous work [35]. We understand that the corresponding energy scales \(\sqrt{eB}\) of the magnetic fields are larger than the energy scale \(\Lambda \) of NJL model, which then seems to invalid these choices of eB. However, if one recognize that NJL model predicts magnetic catalysis effect up to \(eB=4~\mathrm{GeV}^2\) [27] which is qualitatively consistent with LQCD simulations up to \(eB=3.25~\mathrm{GeV}^2\) [52], we have good reason to believe that the valid energy scale is well extended by adopting vacuum regularization. The numerical results are shown in Figs. 3 and 4, respectively. As can be seen in the upper panels, the quark masses all decrease with \(\Omega \) in both cases, but the chiral symmetry restoration (\(\chi \)SR) shows a crossover feature for \(eB=0.5~\mathrm{GeV}^2\) and a first-order one for \(eB=1.5~\mathrm{GeV}^2\). Along with the \(\chi \)SR, the quadratic GL expansion coefficients are evaluated for charged rho meson with both choices of SP in Minkowski space and SP in curved space, see the lower panels in comparison with those of charged pions. For either choice of Schwinger phase, the \(\rho ^\pm \) superconductor can always happen and is favored over the \(\pi ^\pm \) superfluid with large enough \(\Omega \).

Fig. 4
figure4

The evolutions of the dynamical quark masses \(m_{\mathrm{f}}\) (upper panel) and the quadratic GL expansion coefficients \(\mathcal{A}\) (lower panel) with the angular velocity \(\Omega \) at the magnetic field \(eB=1.5~\mathrm{GeV}^2\). The conventions are the same as in Fig. 3

We’ve checked for \(eB=0.5~\mathrm{GeV}^2\) that the \(\pi ^\pm \) superfluid is indeed disfavored with SP in Minkowski space at large \(\Omega \) (\(\ge 0.026~\mathrm{GeV}\)) thus qualitatively consistent with that found in Ref. [38]. But for charged rho meson, the quadratic coefficient keeps decreasing to an order of \(-100~\mathrm{GeV}^2\) at \(\Omega =0.026~\mathrm{GeV}\) without any signature of turning up. The discontinuity in Fig. 4 seems to contradict with the continuous transition assumption in the GL approach, but it surely demonstrates an instability to the \(\chi \)SR phase. The situation might be similar to that of diquark condensation at the critical baryon chemical potential, so here can probably be a first-order transition to \(\rho ^\pm \) superconductor. In the lower panel of Fig. 4, one note that the coefficients \(\mathcal{A}\) increase for charged pion but decrease for charged rho at the critical \(\Omega \ (\sim 8.25~\mathrm{MeV})\). At last, though not illuminated in the plots, it has been checked that the charged axial vector condensation might be favored over \(\chi \)SR or \(\pi ^\pm \) superfluid phase at large enough \(\Omega \) but never over \(\rho ^\pm \) superconductor phase.

Conclusions and discussions

In this work, the possibility of charged rho superconductor in the presence of parallel magnetic field and rotation was intuitively studied in Weinberg model and extensively explored within SU(3) Nambu–Jona-Lasino model. The possibilities of charged \(\pi \) and \(\rho \) condensations in \(\mathbf{B}\parallel \varvec{\Omega }\) both well passed the check in the point particle picture when solely looking at the mesons’ dispersions. By following similar schemes as the previous works on \(\pi ^\pm \) superfluid [37, 38], the \(\rho ^\pm \) superconductor was found to be favored over chiral symmetry breaking, \(\chi \)SR and \(\pi ^\pm \) superfluid phases at large \(\Omega \), for both choices of Schwinger phase in Minkowski and curved spaces. As the chiral partner of \(\rho \) mesons, the charged axial vector meson was even checked in advance; and it turned out that \(\rho ^\pm \) superconductor is still robust against that at large \(\Omega \). Indeed, the NJL model study qualitatively supports the intuitions about the rotation effect on mesons in the point particle approximation.

The present study is not conclusive yet because constant charged rho condensation would contradict the Meissner effect, which excludes the magnetic field out of the superconductor. But the vanishing of the quadratic coefficient should indicate some kind of instability related to \(\rho ^\pm \) condensation [25]. In the future, more realistic but complicated study will be performed to looking for the true ground state of QCD system in \(\mathbf{B}\parallel \varvec{\Omega }\) by taking into account the boundary condition and inhomogeneous forms of condensates consistently [43, 53]. As discussed in Sect. 2, the effective regime of l should be determined by the total energy self-consistently and can be much greater than \({\mathcal {N}}\) for large \(\Omega \). In this case, the \(\pi ^\pm \) superfluid or \(\rho ^\pm \) superconductor is expected to emerge at a smaller threshold of \(\Omega \) compared to what we found here in NJL model. One should notice that: Though \(\rho ^\pm \) superconductor is more favored for the chosen magnetic fields, there is still a window of \(\Omega \) for \(\pi ^\pm \) superfluid when B is relatively weak. Eventually, as the \(\mathbf{B}\parallel \varvec{\Omega }\) is relevant to the circumstance in peripheral HICs, it will be interesting to explore the possible signatures for the competitions among \(\chi \)SR, \(\pi ^\pm \) superfluid and \(\rho ^\pm \) superconductor in experiments.

Data Availability Statement

This manuscript has no associated data or the data will not be deposited. [Authors’ comment: ...].

References

  1. 1.

    V. Skokov, A.Y. Illarionov, V. Toneev, Int. J. Mod. Phys. A 24, 5925 (2009)

    Article  ADS  Google Scholar 

  2. 2.

    W.T. Deng, X.G. Huang, Phys. Rev. C 85, 044907 (2012)

    Article  ADS  Google Scholar 

  3. 3.

    X. Guo, J. Liao, E. Wang, Sci. Rep. 10(1), 2196 (2020)

    Article  ADS  Google Scholar 

  4. 4.

    K. Xu, S. Shi, H. Zhang, D. Hou, J. Liao, M. Huang, Phys. Lett. B 809, 135706 (2020)

    Article  Google Scholar 

  5. 5.

    Z.T. Liang, X.N. Wang, Phys. Rev. Lett. 94, 102301 (2005)

    Article  ADS  Google Scholar 

  6. 6.

    F. Becattini, I. Karpenko, M. Lisa, I. Upsal, S. Voloshin, Phys. Rev. C 95, 054902 (2017)

    Article  ADS  Google Scholar 

  7. 7.

    L. Adamczyk et al., STAR Collaboration. Nature 548, 62 (2017)

  8. 8.

    J. Liao, Pramana 84(5), 901 (2015)

    Article  ADS  Google Scholar 

  9. 9.

    D.E. Kharzeev, J. Liao, S.A. Voloshin, G. Wang, Prog. Part. Nucl. Phys. 88, 1 (2016)

    Article  ADS  Google Scholar 

  10. 10.

    X.G. Huang, Rep. Prog. Phys. 79, 076302 (2016)

    Article  ADS  Google Scholar 

  11. 11.

    J. Adam et al. [STAR Collaboration], arXiv:2006.04251 [nucl-ex]

  12. 12.

    V.P. Gusynin, V.A. Miransky, I.A. Shovkovy, Phys. Rev. Lett. 73, 3499 (1994). Erratum: [Phys. Rev. Lett. 76, 1005 (1996)]

    Article  ADS  Google Scholar 

  13. 13.

    V.P. Gusynin, V.A. Miransky, I.A. Shovkovy, Phys. Lett. B 349, 477 (1995)

    Article  ADS  Google Scholar 

  14. 14.

    I. Karpenko, F. Becattini, Eur. Phys. J. C 77, 213 (2017)

    Article  ADS  Google Scholar 

  15. 15.

    H. Li, L.G. Pang, Q. Wang, X.L. Xia, Phys. Rev. C 96(5), 054908 (2017)

    Article  ADS  Google Scholar 

  16. 16.

    T. Niida [STAR Collaboration], Nucl. Phys. A 982, 511 (2019)

  17. 17.

    Y. Guo, S. Shi, S. Feng, J. Liao, Phys. Lett. B 798, 134929 (2019)

    Article  Google Scholar 

  18. 18.

    G.S. Bali, F. Bruckmann, G. Endrodi, Z. Fodor, S.D. Katz, S. Krieg, A. Schafer, K.K. Szabo, JHEP 1202, 044 (2012)

    Article  ADS  Google Scholar 

  19. 19.

    G.S. Bali, F. Bruckmann, G. Endrodi, Z. Fodor, S.D. Katz, A. Schafer, Phys. Rev. D 86, 071502 (2012)

    Article  ADS  Google Scholar 

  20. 20.

    F. Becattini, I. Karpenko, Phys. Rev. Lett. 120, 012302 (2018)

    Article  ADS  Google Scholar 

  21. 21.

    X.L. Xia, H. Li, Z.B. Tang, Q. Wang, Phys. Rev. C 98, 024905 (2018)

    Article  ADS  Google Scholar 

  22. 22.

    F. Becattini, G. Cao, E. Speranza, Eur. Phys. J. C 79(9), 741 (2019)

    Article  ADS  Google Scholar 

  23. 23.

    X.L. Xia, H. Li, X.G. Huang, H.Z. Huang, Phys. Rev. C 100(1), 014913 (2019)

    Article  ADS  Google Scholar 

  24. 24.

    M.N. Chernodub, Phys. Rev. D 82, 085011 (2010)

    Article  ADS  Google Scholar 

  25. 25.

    M.N. Chernodub, Phys. Rev. Lett. 106, 142003 (2011)

    Article  ADS  Google Scholar 

  26. 26.

    G. Cao, X.G. Huang, Phys. Lett. B 757, 1 (2016)

    Article  ADS  Google Scholar 

  27. 27.

    L. Wang, G. Cao, Phys. Rev. D 97(3), 034014 (2018)

  28. 28.

    L. Wang, G. Cao, X.G. Huang, P. Zhuang, Phys. Lett. B 780, 273 (2018)

    Article  ADS  Google Scholar 

  29. 29.

    G. Cao, Phys. Rev. D 101(9), 094027 (2020)

    MathSciNet  Article  ADS  Google Scholar 

  30. 30.

    Y. Liu, I. Zahed, Phys. Rev. Lett. 120, 032001 (2018)

    Article  ADS  Google Scholar 

  31. 31.

    V.V. Braguta, P.V. Buividovich, M.N. Chernodub, A.Y. Kotov, M.I. Polikarpov, Phys. Lett. B 718, 667 (2012)

  32. 32.

    H. Liu, L. Yu, M. Huang, Phys. Rev. D 91(1), 014017 (2015)

    Article  ADS  Google Scholar 

  33. 33.

    Y. Hidaka, A. Yamamoto, Phys. Rev. D 87(9), 094502 (2013)

    Article  ADS  Google Scholar 

  34. 34.

    G.S. Bali, B.B. Brandt, G. Endrodi, B. Glassle, Phys. Rev. D 97(3), 034505 (2018)

    Article  ADS  Google Scholar 

  35. 35.

    G. Cao, Phys. Rev. D 100(7), 074024 (2019)

    Article  ADS  Google Scholar 

  36. 36.

    H. T. Ding, S. T. Li, S. Mukherjee, A. Tomiya, X. D. Wang, PoS LATTICE2019, 250 (2020)

  37. 37.

    G. Cao, L. He, Phys. Rev. D 100(9), 094015 (2019)

    Article  ADS  Google Scholar 

  38. 38.

    H. L. Chen, X. G. Huang, K. Mameda, arXiv:1910.02700 [nucl-th]

  39. 39.

    C. Vafa, E. Witten, Phys. Rev. Lett. 53, 535 (1984)

    Article  ADS  Google Scholar 

  40. 40.

    H. Zhang, D. Hou, J. Liao, Chin. Phys. C 44(11), 111001 (2020)

    Article  ADS  Google Scholar 

  41. 41.

    S. Weinberg, Phys. Rev. 166, 1568 (1968)

    Article  ADS  Google Scholar 

  42. 42.

    T.D. Lee, C.N. Yang, Phys. Rev. 128, 885 (1962)

    MathSciNet  Article  ADS  Google Scholar 

  43. 43.

    H.L. Chen, K. Fukushima, X.G. Huang, K. Mameda, Phys. Rev. D 96(5), 054032 (2017)

    Article  ADS  Google Scholar 

  44. 44.

    Y. Jiang, J. Liao, Phys. Rev. Lett. 117, 192302 (2016)

    Article  ADS  Google Scholar 

  45. 45.

    P.C.W. Davies, T. Dray, C.A. Manogue, Phys. Rev. D 53, 4382 (1996)

    MathSciNet  Article  ADS  Google Scholar 

  46. 46.

    V.E. Ambrus, E. Winstanley, Phys. Rev. D 93(10), 104014 (2016)

    MathSciNet  Article  ADS  Google Scholar 

  47. 47.

    S.P. Klevansky, Rev. Mod. Phys. 64, 649 (1992)

    MathSciNet  Article  ADS  Google Scholar 

  48. 48.

    S. Klimt, M.F.M. Lutz, U. Vogl, W. Weise, Nucl. Phys. A 516, 429 (1990)

    Article  ADS  Google Scholar 

  49. 49.

    G. ’t Hooft, Phys. Rev. D 14, 3432 (1976) Erratum: [Phys. Rev. D 18, 2199 (1978)]

  50. 50.

    G. Cao, P. Zhuang, Phys. Rev. D 92, 105030 (2015)

    Article  ADS  Google Scholar 

  51. 51.

    P. Rehberg, S.P. Klevansky, J. Hufner, Phys. Rev. C 53, 410 (1996)

    Article  ADS  Google Scholar 

  52. 52.

    G. Endrodi, JHEP 07, 173 (2015)

    Article  ADS  Google Scholar 

  53. 53.

    L. Wang, Y. Jiang, L. He, P. Zhuang, Phys. Rev. D 100(11), 114009 (2019)

    MathSciNet  Article  ADS  Google Scholar 

Download references

Acknowledgements

We thank Jinfeng Liao for helpful discussions. G.C. is supported by the National Natural Science Foundation of China with Grant No. 11805290 and Young Teachers Training Program of Sun Yat-sen University with Grant No. 19lgpy282.

Author information

Affiliations

Authors

Corresponding author

Correspondence to Gaoqing Cao.

Rights and permissions

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

Funded by SCOAP3

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Cao, G. Charged rho superconductor in the presence of magnetic field and rotation. Eur. Phys. J. C 81, 148 (2021). https://doi.org/10.1140/epjc/s10052-021-08900-8

Download citation