This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

Correlations of net baryon number and electric charge in nuclear matter

Xin-ran Yang School of Physics, Xi’an Jiaotong University, Xi’an, 710049, China MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Xi’an Jiaotong University, Xi’an, 710049, China    Guo-yun Shao [email protected] School of Physics, Xi’an Jiaotong University, Xi’an, 710049, China MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Xi’an Jiaotong University, Xi’an, 710049, China    Chong-long Xie School of Physics, Xi’an Jiaotong University, Xi’an, 710049, China MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Xi’an Jiaotong University, Xi’an, 710049, China    Zhi-Peng Li School of Physics, Xi’an Jiaotong University, Xi’an, 710049, China MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Xi’an Jiaotong University, Xi’an, 710049, China
Abstract

Abstract: We investigate the correlations between net baryon number and electric charge up to sixth order related to the interactions of nuclear matter at low temperature, and explore their relationship with the nuclear liquid-gas phase transition (LGPT) within the framework of the nonlinear Walecka model. The calculation shows that strong correlations between the baryon number and electric charge exist in the vicinity of LGPT, and the higher order correlations are more sensitive than the lower order ones near the phase transition. However, in the high-temperature region away from the LGPT the rescaled lower order correlations are relatively larger than most of the higher order ones. Besides, some of the fifth- and sixth-order correlations possibly change the sign from negative to positive along the chemical freeze-out line with the decrease of temperature. In combination with the future experimental projects at lower collision energies, the derived results can be referred to study the phase structure of strongly interacting matter and analyze the related experimental signals.

Keywords: Correlations of conserved charges, Nuclear matter, Nuclear liquid-gas phase transition, Heavy-ion collision

I introduction

One of the primary goals in nuclear physics is to map the phase diagram of quantum chromodynamics (QCD). It involves the chiral and deconfinement phase transtions related to the transformation from quark-gluon plasma to hadronic matter Shou24 . The calculations from lattice QCD and hadron resonance gas  (HRG) model indicate that a smooth crossover tranformation occurs at high temperature and small chemical potential Aoki06 ; Bazavov19 ; Borsanyi13 ; Bazavov14 ; Bazavov17 ; Borsanyi14 ; Borsanyi20 . Moreover, many studies in the effective quark models (e.g., Ref.Fukushima04 ; Ratti06 ; Costa10 ; Fu08 ; Sasaki12 ; Ferreira14 ; Shao2018 ; Schaefer10 ; Skokov11 ; Liu2018 ; Chen20 ; Zhao23 ; Ferreira2018 ; Yang24 ), the Dyson-Schwinger equation approach Gao24 ; Qin11 ; Gao16 ; Gao20 ; Fischer14 ; Shi14 , the functional renormalization group theory Fu20 ; Rennecke17 ; Fu21 and machine learning Ma23 , suggest that a first-order chiral phase transition undergoes at large chemical potential.

Fluctuations and correlations of conserved charges ( baryon number BB, electric charge QQ and strangeness SS) are sensitive observables to study the phase transition of strongly interacting matter Stephanov . The net proton (proxy of net baryon) cumulants have been measured in the beam energy scan (BES) program at the Relativistic Heavy Ion Collider (RHIC) Aggarwal10 ; Adamczyk14 ; Chen24 ; Luo2017 ; Aboona23 ; Zhang23 ; Chen23 , which has sparked extensive study about QCD phase transition, in particular, the QCD critical endpoint (CEP). More impressively, the distributions of net proton number at the center-of mass energy sNN=3\sqrt{s_{NN}}=3 and 2.42.4\,GeV are essentially different from those at 7.77.7\,GeV and above, since the fluctuation distributions of net proton number are primarily dominated by the interaction among hadrons Aboona23 .

The experimental results at 33\,GeV and below raise the question of how the hadronic interactions affect the fluctuations of conserved charges at lower-energy regimes Huang23 ; ShaoJ23 ; Marczenko23 ; Liu22 . With the decrease of collision energy, the nuclear liquid-gas phase transition (LGPT) is possibly involved He23 ; Shao20 ; Chomaz04 ; Pochodzalla95 ; Borderie01 ; Botvina95 ; Agostino99 ; Srivastava02 ; Elliott02 ; Xu2023 ; Ma1999 ; Deng2022 ; Hempel13 ; Mukherjee17 ; Xu13 ; Savchuk20 ; Wang20 . In Ref. Poberezhnyuk19 ; Vovchenko17 ; Poberezhnyuk21 , a van der Waals model was used to study the high-order distributions of net baryon number in both the pure and mixed phases of the LGPT. In Ref. Marczenko23 , the second-order susceptibility of net baryon number for positive- and negative-parity nucleons was examined near the chiral and nuclear liquid-gas phase transitions using the double parity model, in which both the chiral phase transition and nuclear LGPT are effectively included. In Ref. Shao20 ; Xu2023 , the net baryon kurtosis and skewness were considered in the non-linear Walecka model to analyze the experimental signals at lower collision energies. The hyperskewness and hyperkurtosis of net baryon number were further calculated recently to explore the relation between nuclear LGPT and experimental observables Yang2024 .

Since the interactions among hadrons dominate the density fluctuations at lower energy regimes (below 33\,GeV), the BES program at collision energies lower than 7.77.7\,GeV will provide more information about the phase structure of strongly interacting matter. The relevant experiments are also in plan at High Intensity heavy-ion Accelerator Facility (HIAF). Meanwhile, the HADES collaboration at GSI Helmholtzzentrum für Schwerionenforschung planned to measure higher-order net proton and net charge fluctuations in central Au + Au reactions at collision energies ranging from 0.2A0.2A to 1.0A1.0A\,GeV to probe the LGPT region Bluhm20 . These experiments are significant for investigating the nuclear liquid-gas and chiral phase transitions through the density fluctuations.

Besides the fluctuations of conserved charges, the correlations of different conserved charges can also provide important information to explore the phase transition. The correlations of conserved charges or the off-diagonal susceptibilities have been calculated to study the chiral and deconfinement phase transitions at high temperature in lattice QCD and some effective quark models (e.g., Bellwied15 ; Wen2021 ; Ding2015 ; Fodor18 ; Bellwied20 ; Fu10 ; Bhattacharyya11 ). However, the correlations of net baryon number and electric charge in nuclear matter and their relationship with nuclear LGPT are still absent, which are useful in diagnosing the phase diagram of strongly interacting matter at low temperature. In this study, we will explore the correlations between net baryon number and electric charge up to sixth order in nuclear matter using the nonlinear Walecka model. Some characteristic behaviors of correlations evoked by the nucleon-nucleon interaction near and far away from the nuclear LGPT are obtained. These results will help analyze the chiral phase transition, nuclear LGPT and the related experimental signals in the future.

The paper is organized as follows. In Sec. II, we introduce the formulas to describe correlations of conserved charges and the nonlinear Walecka model. In Sec. III, we illustrate the numerical results of correlations of net baryon number and electric charge. A summary is finally given in Sec. IV.

II Correlations of conserved charges and the nonlinear Walecka model

The fluctuations and correlations of conserved charges are related to the equation of state of a thermodynamic system. In the grand-canonical ensemble of strongly interacting matter the pressure is the logarithm of partition function Karsch15 :

P=TVlnZ(V,T,μB,μQ,μS),P=\frac{T}{V}\ln{Z(V,T,\mu_{B},\mu_{Q},\mu_{S})}, (1)

where μB,μQ,μS\mu_{B},\mu_{Q},\mu_{S} are the chemical potentials of conserved charges, i.e., the baryon number, electric charge and strangeness in strong interaction, respectively. The generalized susceptibilities can be derived by taking the partial derivatives of the pressure with respect to the corresponding chemical potentials Luo2017

χijkBQS=i+j+k[P/T4](μB/T)i(μQ/T)j(μS/T)k.\chi^{BQS}_{ijk}=\frac{\partial^{i+j+k}[P/T^{4}]}{\partial(\mu_{B}/T)^{i}\partial(\mu_{Q}/T)^{j}\partial(\mu_{S}/T)^{k}}. (2)

In experiments, the cumulants of multiplicity distributions of the conserved charges are usually measured. They are related to the generalized susceptibilities by

CijkBQS=i+j+kln[Z(V,T,μB,μQ,μS)](μB/T)i(μQ/T)j(μS/T)k=VT3χijkBQS.\!C^{BQS}_{ijk}\!=\!\frac{\partial^{i\!+\!j\!+\,k}\ln[Z(V,T,\mu_{B},\mu_{Q},\mu_{S})]}{\partial(\mu_{B}/T)^{i}\partial(\mu_{Q}/T)^{j}\partial(\mu_{S}/T)^{k}}\!=\!V\!T^{3}\chi^{BQS}_{ijk}\,. (3)

To eliminate the volume dependence in heavy-ion collision experiments, observables are usually constructed by the ratios of cumulants, and then can be compared with the theoretical calculations of the generalized susceptibilities with

CijkBQSClmnBQS=χijkBQSχlmnBQS.\frac{C^{BQS}_{ijk}}{C^{BQS}_{lmn}}=\frac{\chi^{BQS}_{ijk}}{\chi^{BQS}_{lmn}}. (4)

In this research the nonlinear Walecka model is taken to calculate the correlations of net baryon number and electric charge in nuclear matter at low temperature. This model is generally used to describe the properties of finite nuclei and the equation of state of nuclear matter. The approximate equivalence of this model to the hadron resonance gas model at low temperature and small density was also indicated in Ref. Fukushima15 . This model was recently taken to explore the fluctuations of net baryon number in nuclear matter, e.g., the kurtosis and skewness in Ref. Shao20 ; Xu2023 , and the hyperskewness and hyperkurtosis Yang2024 .

The Lagrangian density for the nucleons-meson system in the nonlinear Walecka model Glendenning97 ; He23 is

\displaystyle\cal{L}\! =\displaystyle\!=\! Nψ¯N[iγμμ(mNgσσ)gωγμωμgργμ𝝉𝝆μ]ψN\displaystyle\sum_{N}\bar{\psi}_{N}\!\big{[}i\gamma_{\mu}\partial^{\mu}\!-\!(\!m_{N}\!-\!g_{\sigma}\sigma)\!\!-\!g_{\omega}\gamma_{\mu}\omega^{\mu}\!-\!g_{\rho}\!\gamma_{\mu}\boldsymbol{\tau}\!\cdot\!\boldsymbol{\rho}^{\mu}\big{]}\!\psi_{N} (5)
+12(μσμσmσ2σ2)13bmN(gσσ)314c(gσσ)4\displaystyle+\frac{1}{2}\left(\partial_{\mu}\sigma\partial^{\mu}\sigma-m_{\sigma}^{2}\sigma^{2}\right)\!-\!\frac{1}{3}bm_{N}\,(g_{\sigma}\sigma)^{3}-\frac{1}{4}c\,(g_{\sigma}\sigma)^{4}
+12mω2ωμωμ14ωμνωμν\displaystyle+\frac{1}{2}m^{2}_{\omega}\omega_{\mu}\omega^{\mu}-\frac{1}{4}\omega_{\mu\nu}\omega^{\mu\nu}
+12mρ2𝝆μ𝝆μ14𝝆μν𝝆μν,\displaystyle+\frac{1}{2}m^{2}_{\rho}\boldsymbol{\rho}_{\mu}\!\cdot\!\boldsymbol{\rho}^{\mu}\!-\!\frac{1}{4}\boldsymbol{\rho}_{\mu\nu}\!\cdot\!\boldsymbol{\rho}^{\mu\nu},

where ωμν=μωννωμ\omega_{\mu\nu}=\partial_{\mu}\omega_{\nu}-\partial_{\nu}\omega_{\mu}, ρμν=μ𝝆νν𝝆μ\rho_{\mu\nu}=\partial_{\mu}\boldsymbol{\rho}_{\nu}-\partial_{\nu}\boldsymbol{\rho}_{\mu} and mNm_{N} is the nucleon mass in vacuum. The interactions between nucleons are mediated by σ,ω,ρ\sigma,\,\omega,\,\rho mesons..

The thermodynamic potential can be derived in the mean-field approximation

Ω=\displaystyle\Omega=\! β1N2d3𝒌(2π)3[ln(1+eβ(EN(k)μN))\displaystyle\!-\!\beta^{-1}\sum_{N}2\!\int\frac{d^{3}\boldsymbol{k}}{(2\pi)^{3}}\!\bigg{[}\ln\!\left(1+e^{-\beta\left(E_{N}^{*}(k)-\mu_{N}^{*}\!\right)}\right)\! (6)
+ln(1+eβ(EN(k)+μN))]+12mσ2σ2+13bmN(gσσ)3\displaystyle+\!\ln\!\left(1\!+\!e^{-\beta\left(E_{N}^{*}(k)+\mu_{N}^{*}\right)}\right)\!\bigg{]}\!+\!\frac{1}{2}m_{\sigma}^{2}\sigma^{2}\!+\!\frac{1}{3}bm_{N}\left(g_{\sigma}\sigma\right)^{3}
+14c(gσσ)412mω2ω212mρ2ρ32,\displaystyle+\frac{1}{4}c\left(g_{\sigma}\sigma\right)^{4}-\frac{1}{2}m_{\omega}^{2}\omega^{2}-\frac{1}{2}m_{\rho}^{2}\rho_{3}^{2},

where β=1/T\beta=1/T, EN=k2+mN2E_{N}^{*}=\sqrt{k^{2}+m_{N}^{*2}}, and ρ3\rho_{3} is the third component of ρ\rho meson field. The effective nucleon mass mN=mNgσσm^{*}_{N}=m_{N}-g_{\sigma}\sigma and the effective chemical potential μN\mu_{N}^{*} is defined as μN=μNgωωτ3Ngρρ3\mu_{N}^{*}=\mu_{N}-g_{\omega}\omega-\tau_{3N}g_{\rho}\rho_{3} (τ3N=1/2\tau_{3N}=1/2 for proton, 1/2-1/2 for neutron).

By minimizing the thermodynamical potential

Ωσ=Ωω=Ωρ3=0,\frac{\partial\Omega}{\partial\sigma}=\frac{\partial\Omega}{\partial\omega}=\frac{\partial\Omega}{\partial\rho_{3}}=0, (7)

the meson field equations can be derived as

gσσ=(gσmσ)2[ρps+ρnsbmN(gσσ)2c(gσσ)3],g_{\sigma}\sigma\!=\!\left(\frac{g_{\sigma}}{m_{\sigma}}\right)^{2}\!\left[\rho_{p}^{s}+\rho_{n}^{s}-bm_{N}\left(g_{\sigma}\sigma\right)^{2}-c\left(g_{\sigma}\sigma\right)^{3}\right], (8)
gωω=(gωmω)2(ρp+ρn),g_{\omega}\omega=\left(\frac{g_{\omega}}{m_{\omega}}\right)^{2}\left(\rho_{p}+\rho_{n}\right), (9)
gρρ3=12(gρmρ)2(ρpρn).g_{\rho}\rho_{3}=\frac{1}{2}\left(\frac{g_{\rho}}{m_{\rho}}\right)^{2}\left(\rho_{p}-\rho_{n}\right). (10)

In Eqs.(8)-(10), the nucleon number density

ρi=2d3𝒌(2π)3[f(Eiμi)f¯(Ei+μi)],\rho_{i}=2\int\frac{d^{3}\boldsymbol{k}}{(2\pi)^{3}}[f\left(E_{i}^{*}-\mu_{i}^{*}\right)-\bar{f}\left(E_{i}^{*}+\mu_{i}^{*}\right)], (11)

and the scalar density

ρis=2d3𝒌(2π)3miEi[f(Eiμi)+f¯(Ei+μi)],\rho_{i}^{s}=2\int\frac{d^{3}\boldsymbol{k}}{(2\pi)^{3}}\frac{m_{i}^{*}}{E_{i}^{*}}[f\left(E_{i}^{*}-\mu_{i}^{*}\right)+\bar{f}\left(E_{i}^{*}+\mu_{i}^{*}\right)], (12)

where f(Eiμi)f(E_{i}^{*}-\mu_{i}^{*}) and f¯(Ei+μi)\bar{f}(E_{i}^{*}+\mu_{i}^{*}) are the fermion and antifermion distribution functions with

f(Eiμi)=11+exp{[Eiμi]/T},f(E_{i}^{*}-\mu_{i}^{*})=\frac{1}{1+\exp\left\{\left[E_{i}^{*}-\mu_{i}^{*}\right]/T\right\}}, (13)

and

f(Ei+μi)=11+exp{[Ei+μi]/T}.f(E_{i}^{*}+\mu_{i}^{*})=\frac{1}{1+\exp\left\{\left[E_{i}^{*}+\mu_{i}^{*}\right]/T\right\}}. (14)

The meson field equations can be solved for a given temperature and chemical potential (or baryon number density). The model parameters, gσ,gω,gρ,bg_{\sigma},g_{\omega},g_{\rho},b and cc, are listed in Table. 1. They are fitted with the compression modulus K=240K=240\,MeV, the symmetric energy asym=31.3a_{sym}=31.3\,MeV, the effective nucleon mass mN=mNgσσ=0.75mNm^{*}_{N}=m_{N}-g_{\sigma}\sigma=0.75m_{N} and the binding energy B/A=16.0B/A=-16.0\,MeV at nuclear saturation density with ρ0=0.16fm3\rho_{0}=0.16\,fm^{-3}.

Table 1: Parameters in the nonlinear Walecka model
(gσ/mσ)2\left({g_{\sigma}}/{m_{\sigma}}\right)^{2}/fm2 (gω/mω)2\left({g_{\omega}}/{m_{\omega}}\right)^{2}/fm2 (gρ/mρ)2\left({g_{\rho}}/{m_{\rho}}\right)^{2}/fm2 bb cc
10.32910.329 5.423 0.95 0.00692 -0.0048

III numerical results and discussions

In this section, we present the numerical results of the correlations between net baryon number and electric charge in the non-linear Walecka model. To simulate the physical conditions in the BES program at RHIC STAR, the isospin asymmetric nuclear matter is considered in the calculation with the constraint of ρQ/ρB=0.4\rho_{Q}/\rho_{B}=0.4. In the present Walecka model, strange baryons are not included, thus the strangeness condition of ρS=0\rho_{S}=0 is automatically satisfied. Note that ρQ/ρB=0.4\rho_{Q}/\rho_{B}=0.4 might be slightly deviated due to isospin dynamics. We will detailedly explore the influence of different isospin asymmetries on the fluctuations and correlations of conserved charges in a separate study.

Refer to caption
Figure 1: Contour of μQ\mu_{Q} in the TμBT-\mu_{B} plane derived in the nonlinear Walecka model with the constraint of ρQ/ρB=0.4\rho_{Q}/\rho_{B}=0.4. The solid line is the liquid-gas transition line with a CEP locating at T=13T=13\,MeV and μB=919\mu_{B}=919\,MeV. The blue line is the chemical freeze-out line fitted in Ref. Cleymans06 . The dash-dotted line corresponds to the temperature and chemical potential for ρB=0.1ρ0\rho_{B}=0.1\rho_{0}. “Line A” is derived with σ/μB\partial\sigma/\partial\mu_{B} taking the maximum value for each given temperature.

The correlations between baryon number and electric charge are related to the baryon chemical potential μB\mu_{B} and isospin chemical potential μQ\mu_{Q} (μQ=μpμn\mu_{Q}=\mu_{p}-\mu_{n}). To demonstrate the value of μQ\mu_{Q} as a function of temperature and baryon chemical potential, we first plot in Fig. 1 the contour map of μQ\mu_{Q} in the TμBT-\mu_{B} plane derived under the constraint of ρQ/ρB=0.4\rho_{Q}/\rho_{B}=0.4. The corresponding liquid-gas phase transition line with a CEP locating at T=13T=13\,MeV and μB=919\mu_{B}=919\,MeV is also plotted in this figure. To compare with the chiral crossover phase transition of quarks, the dashed line labeled as “Line A” in Fig. 1 is derived with the condition that σ/μB\partial\sigma/\partial\mu_{B} takes the maximum value for each given temperature. This line plays a role analogous in a certain degree to the chiral crossover transformation, although it is not a true phase transition in nuclear matter. It indicates the location where the dynamical nucleon mass changes most quickly with the increase of chemical potential. The reason for this is to emphasize that both the σ\sigma field in nuclear matter and quark condensate in quark matter are associated with the dynamical mass of fermions and, therefore the rapid change of mass might have the universal effect on fluctuation distributions of conserved charges. As pointed out in our previous studies He2023; Shao20 ; Yang2024 , the location of line A helps understand the behaviors of interaction measurement (trace anomaly), the fluctuations of conserved charges near the phase transition Shao20 ; Yang2024 .

One can also define “Line A” by the maximum point of ω/μB\partial\omega/\partial\mu_{B} or nB/μB\partial n_{B}/\partial\mu_{B}, since the density can be taken as the order parameter for liquid-gas phase transition. Under this definition, the result obtained in quark model does not correspond to the chiral crossover phase transition. This is not the purpose of this study. Our aim is to indicate some common properties related to dynamical fermion mass near the critical region of a first-order phase transition. On the other hand, the calculation indicates that the curves (“Line A”) under the two definitions coincide near the critical region, and the two curves gradually deviate at higher temperatures away from the critical region.

For the convenience of subsequent discussion of experimental observables, we also plot in Fig. 1 the chemical freeze-out line fitted with experimental data at high energies Cleymans06 , which can be described with

T(μB)=abμB2cμB4,T\left(\mu_{B}\right)=a-b\mu_{B}^{2}-c\mu_{B}^{4}, (15)

where a=0.166GeV,b=0.139GeV1a=0.166\,\mathrm{GeV},b=0.139\,\mathrm{GeV}^{-1} and c=0.053GeV3c=0.053\,\mathrm{GeV}^{-3}. We should remind that the trajectories of the present relativistic heavy-ion collisions do not pass through the TCT_{C} of nuclear LGPT. It is still not known how far the realistic chemical freeze-out line is from the critical region in future experiments. However, similar to the chiral phase transition of quarks, the existence of nuclear LGPT affects the fluctuation and correlation of net baryon and electric charge number in the region not very adjacent to the critical end point in intermediate-energy heavy-ion collision experiments. The numerical results on the parameterized chemical freeze-out line in this study can be taken as a reference. The realistic chemical freeze-out condition at intermediate and low energies will be extracted in future heavy-ion collision experiments. When analyzing the experimental data the contribution from LGPT needs to be considered.

Fig. 1 shows that the value of |μQ|\left|\mu_{Q}\right| is smaller than 4040\,MeV in the area covered in red. In this region the baryon number density is very small, which can be seen roughly from the temperature and chemical potential curve for ρB=0.1ρ0\rho_{B}=0.1\rho_{0} (dash-dotted line). The value of |μQ|\left|\mu_{Q}\right| increases with the rising baryon density (corresponding to larger chemical potential). This trend of |μQ|\left|\mu_{Q}\right| is clearly illustrated in Fig. 1. Along the chemical freeze-out line (solid blue line), one can see how μQ\mu_{Q} changes at freeze-out with the decrease of temperature or collision energy.

Refer to caption
Figure 2: Second order correlation between baryon number and electric charge as a function of chemical potential for different temperatures. The solid dots demonstrate the values on the chemical freeze-out line given in Fig. 1.

We demonstrate in Fig. 2 the second order correlation between baryon number and electric charge, χ11BQ/χ2Q\chi_{11}^{BQ}/\chi_{2}^{Q}, as functions of baryon chemical potential for T=75,50,25T=75,50,25\,MeV, respectively. To derive the physical quantity comparable with future experiments the correlated susceptibility is divided by χ2Q\chi_{2}^{Q}, which eliminates the volume dependence. For each temperature, the rescaled second-order correlation χ11BQ/χ2Q\chi_{11}^{BQ}/\chi_{2}^{Q} in Fig. 2 displays a nonmonotonic behavior with a peak structure at a certain chemical potential. The values of these peaks increase with the decline of temperature, which indicate the correlation between baryon number and electric charge is enhanced near the phase transition region. The solid dots in Fig. 2 demonstrate the values at chemical freeze-out described by Eq. (15), which illustrate that the value of χ11BQ/χ2Q\chi_{11}^{BQ}/\chi_{2}^{Q} increases along the freeze-out line when moving from the high-temperature side to the critical region.

Refer to caption
Refer to caption
Refer to caption
Figure 3: Third order correlations between baryon number and electric charge as functions of chemical potential at different temperatures. The solid dots demonstrate the values on the chemical freeze-out line plotted in Fig. 1.

Fig. 3 shows the third order correlations, χ12BQ/χ2Q\chi_{12}^{BQ}/\chi_{2}^{Q} and χ21BQ/χ2Q\chi_{21}^{BQ}/\chi_{2}^{Q}, as functions of chemical potential for several temperatures. Compared with the χ12BQ/χ2Q\chi_{12}^{BQ}/\chi_{2}^{Q}, the fluctuation of χ21BQ/χ2Q\chi_{21}^{BQ}/\chi_{2}^{Q} is relatively larger at the same temperature. The solid dots at chemical freeze-out line present the same trend. This means the measurement of χ21BQ/χ2Q\chi_{21}^{BQ}/\chi_{2}^{Q} is more sensitive than χ12BQ/χ2Q\chi_{12}^{BQ}/\chi_{2}^{Q} in heavy-ion collision experiments. Fig. 3 also indicates that with the decrease of temperature, the correlations between baryon number and electric charge intensify. An evident oscillations of χ12BQ/χ2Q\chi_{12}^{BQ}/\chi_{2}^{Q} and χ21BQ/χ2Q\chi_{21}^{BQ}/\chi_{2}^{Q} appear for T=25T=25\,MeV, accompanied by the alternating positives and negatives. With the decrease of temperature, the divergent behavior appears at the CEP of LGPT. These features can be used to look for the signal of phase transition in experiments.

Refer to caption
Refer to caption
Refer to caption
Figure 4: Fourth order correlations between baryon number and electric charge as functions of chemical potential for different temperatures. The solid dots demonstrate the values on the chemical freeze-out line given in Fig. 1.
Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 5: Fifth order correlations between baryon number and electric charge as functions of chemical potential for different temperatures. The solid dots demonstrate the values on the chemical freeze-out line given in Fig. 1.

In Fig. 4, we plot the fourth order correlations between baryon number and electric charge, χ13BQ/χ2Q\chi_{13}^{BQ}/\chi_{2}^{Q}, χ22BQ/χ2Q\chi_{22}^{BQ}/\chi_{2}^{Q} and χ31BQ/χ2Q\chi_{31}^{BQ}/\chi_{2}^{Q}. Compared with the second and third order correlations in Fig. 2 and Fig. 3, Fig. 4 shows that the rescaled fourth order correlations by χ2Q\chi_{2}^{Q} are weaker at higher temperature, e.g., T=75T=75\,MeV. However, the correlations are much stronger at T=25T=25\,MeV, near the critical region of LGPT. Correspondingly, there is evidently a bimodal structure for all the three correlations with the increase of chemical potential at lower temperature. It is also seen that the maximum values of χ13BQ/χ2Q\chi_{13}^{BQ}/\chi_{2}^{Q}, χ22BQ/χ2Q\chi_{22}^{BQ}/\chi_{2}^{Q} and χ31BQ/χ2Q\chi_{31}^{BQ}/\chi_{2}^{Q} increase in turn. Besides, the solid dots demonstrate the value of each correlation at freeze-out increases with the decline of temperature. Moreover, it is seen that χ13BQ/χ2Q<χ22BQ/χ2Q<χ31BQ/χ2Q\chi_{13}^{BQ}/\chi_{2}^{Q}<\chi_{22}^{BQ}/\chi_{2}^{Q}<\chi_{31}^{BQ}/\chi_{2}^{Q} at chemical freeze-out for each temperature. It implies that χ31BQ/χ2Q\chi_{31}^{BQ}/\chi_{2}^{Q} is most sensitive among the three fourth-order correlations.

Fig. 5 presents the fifth order correlations between baryon number and electric charge, χ14BQ/χ2Q\chi_{14}^{BQ}/\chi_{2}^{Q}, χ23BQ/χ2Q\chi_{23}^{BQ}/\chi_{2}^{Q} χ32BQ/χ2Q\chi_{32}^{BQ}/\chi_{2}^{Q} and χ41BQ/χ2Q\chi_{41}^{BQ}/\chi_{2}^{Q} for T=75,50,25T=75,50,25\,MeV. This figure shows that at T=75T=75\,MeV, the values of the three rescaled correlations are all quite small, but they become drastic at T=25T=25\,MeV. In combination with the phase diagram in Fig. 1, it can been seen that the closer they get to the liquid-gas transition the stronger the high-order correlated fluctuations. Similar to the fourth order correlations, the rescaled fifth correlations fullfill the relations of |χ14BQ/χ2Q|<|χ23BQ/χ2Q|<|χ32BQ/χ2Q|<|χ41BQ/χ2Q|\left|\chi_{14}^{BQ}/\chi_{2}^{Q}\right|<\left|\chi_{23}^{BQ}/\chi_{2}^{Q}\right|<\left|\chi_{32}^{BQ}/\chi_{2}^{Q}\right|<\left|\chi_{41}^{BQ}/\chi_{2}^{Q}\right| at chemical freeze-out. Moreover, a remarkable result is that all the four fifth-order correlation fluctuations are negative at chemical freeze-out for T=75T=75 and 5050\,MeV, but they are positive at T=25T=25\,MeV, close to the region of liquid-gas transition. This is a prominent feature in exploring the interaction and phase transition of nuclear matter.

Fig. 6 shows the sixth order correlations of baryon number and electric charge, ie., χ15BQ/χ2Q\chi_{15}^{BQ}/\chi_{2}^{Q}, χ24BQ/χ2Q\chi_{24}^{BQ}/\chi_{2}^{Q} χ33BQ/χ2Q\chi_{33}^{BQ}/\chi_{2}^{Q}, χ42BQ/χ2Q\chi_{42}^{BQ}/\chi_{2}^{Q} and χ51BQ/χ2Q\chi_{51}^{BQ}/\chi_{2}^{Q}. Each of the sixth order correlations has a double-peak and double-valley structure, although one of the two peaks is not prominent. It is seen that the oscillating behavior intensifies when moving towards the phase transition region from high temperatures to lower ones. Similarly, the intensity of oscillations increases in turn from χ15BQ/χ2Q\chi_{15}^{BQ}/\chi_{2}^{Q}, χ24BQ/χ2Q\chi_{24}^{BQ}/\chi_{2}^{Q} χ33BQ/χ2Q\chi_{33}^{BQ}/\chi_{2}^{Q}, χ42BQ/χ2Q\chi_{42}^{BQ}/\chi_{2}^{Q} to χ51BQ/χ2Q\chi_{51}^{BQ}/\chi_{2}^{Q}.

For a given order of correlations, the numerical results in Fig. 2-6 show that the signals become stronger when there are more derivatives with respect to baryon chemical potential than that with to electric chemical potential. We also checked the pure baryon number fluctuation, and found it is the most sensitive one at the same order to the LGPT critical end point. The possible reason is that the baryon number fluctuation includes both the proton and neutron’s contribution. However, the electric charge fluctuation involves the isospin density, ρNρP\rho_{N}-\rho_{P}. The baryon number density is always larger than the isospin density, which is associated with stronger fluctuations when there are more derivatives with respect to baryon chemical potential than that with to electric chemical potential for a given order of correlations.

Additionally, comparing the results in Fig. 2-6, we can find that the rescaled higher-order correlations fluctuate more strongly near the phase transition region, while the lower-order correlations at high temperature are relatively larger than most of the higher-order ones away from the phase transition region. The similar phenomenon exist for the correlations of conserved charges in quark matter Fu10 . According to the fluctuations of net baryon number Shao20 ; Yang2024 , and the correlations between net baryon number and electric charge in this study, it can be seen that the fluctuations and correlations of conserved charges have similar organization structures for nuclear and quark matter. This can be mainly attributed to that the two phase transitions belong to the same universal class and they both describe the interacting matter with temperature and chemical potential dependent fermion masses.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 6: Sixth order correlations between baryon number and electric charge as functions of chemical potential for different temperatures. The solid dots demonstrate the values on the chemical freeze-out line given in Fig. 1.

Since the QCD phase transition and nuclear LGPT possibly occur sequentially form high to low temperature, (even if the LGPT is not triggered) the energy dependent behaviors of fluctuations and correlations can be referenced to look for the phase transition signals of strongly interacting matter. Although the latest reported BES II high-precision data at 7.7397.7-39\,GeV does not show a drastic change of the net baryon number kurtosis, the stronger fluctuation signals possibly appear in heavy-ion experiments with collision energies lower than 7.77.7 GeV. Furthermore, in the hadronic interaction dominant evolution with collision energies lower than the threshold of the generation of QGP, the nuclear interaction and phase structure of LGPT will dominate the behavior of fluctuations and correlations of conserved charges. It is worth looking forward to how the fluctuations and correlations change in experiments with the decrease of collision energy.

IV summary and conclusion

Fluctuations and correlations of conserved charges are sensitive probes to investigate the phase structure of strongly interacting matter. In this research, we calculated the correlations between net baryon number and electric charge up to sixth order caused by the hadronic interactions in nuclear matter with the non-linear Walecka model, and explored how they relate to nuclear liquid-gas phase transition.

The calculation indicates that the correlations between net baryon number and electric charge gradually become stronger from the high-temperature region to critical region of nuclear LGPT. In particular, the correlations are drastic at the location where the σ\sigma field or nucleon mass changes rapidly near the critical region. A similar behavior exists for the chiral crossover phase transition of quark matter. This is mainly attributed to the similar dynamical mass evolution and the same universal class for the chiral phase transition of quark matter and the liquid-gas phase transition of nuclear matter.

Compared with the lower order correlations, the higher order correlations fluctuate more strongly near the phase transition region, while the rescaled lower order correlations are relatively stronger than most of the higher-order ones away from the phase transition region at high temperature. At the chemical freeze-out for each temperature, the calculation shows χ13BQ/χ2Q<χ22BQ/χ2Q<χ31BQ/χ2Q\chi_{13}^{BQ}/\chi_{2}^{Q}<\chi_{22}^{BQ}/\chi_{2}^{Q}<\chi_{31}^{BQ}/\chi_{2}^{Q} for the fourth order correlation, |χ14BQ/χ2Q|<|χ23BQ/χ2Q|<|χ32BQ/χ2Q|<|χ41BQ/χ2Q||\chi_{14}^{BQ}/\chi_{2}^{Q}|<|\chi_{23}^{BQ}/\chi_{2}^{Q}|<|\chi_{32}^{BQ}/\chi_{2}^{Q}|<|\chi_{41}^{BQ}/\chi_{2}^{Q}| for the fifth order correlations, and |χ15BQ/χ2Q|<|χ24BQ/χ2Q|<|χ33BQ/χ2Q|<|χ42BQ/χ2Q|<|χ51BQ/χ2Q||\chi_{15}^{BQ}/\chi_{2}^{Q}|<|\chi_{24}^{BQ}/\chi_{2}^{Q}|<|\chi_{33}^{BQ}/\chi_{2}^{Q}|<|\chi_{42}^{BQ}/\chi_{2}^{Q}|<|\chi_{51}^{BQ}/\chi_{2}^{Q}| for the sixth order correlations. In particular, the values of fifth and sixth order correlations change from negative to positive when approaching to the critical region of LGPT from the high-temperature side along the extrapolated chemical freeze-out line. With the release of more precise data in experiments below 7.7 GeV in the future, the realistic chemical freeze-out condition can be fitted and the results obtained in this research can be referred to analyze the signals of QCD phase transition and the influence of nuclear liquid-gas phase transition.

Acknowledgements

This work is supported by the National Natural Science Foundation of China under Grant No. 12475145, 11875213, and the Natural Science Basic Research Plan in Shaanxi Province of China (Program No. 2024JC-YBMS-018).

References

References

  • (1) Q. Y. Shou, Y. G Ma, S. Zhang, et al., Nucl. Sci. Tech. 35, 219 (2024).
  • (2) Y. Aoki, G. Endrodi, Z. Fodor, S. D. Katz, and K. K. Szabo, Nature 443, 675 (2006).
  • (3) A. Bazavov H. T. Ding b, P. Hegde, O. Kaczmarek, F. Karsch, N. Karthiks, et al., (hotQCD Collaboration) Phys. Lett. B 795, 15 (2019).
  • (4) S. Borsányi, Z. Fodor, S. D. Katz, S. Krieg, C. Ratti, and K. K. Szabó, Phys. Rev. Lett. 111, 062005 (2013).
  • (5) A. Bazavov, et al., (hotQCD Collaboration), Phys. Rev. D. 90, 094503 (2014).
  • (6) A. Bazavov, et al., (hotQCD Collaboration), Phys. Rev. D 96, 074510 (2017).
  • (7) S. Borsányi, Z. Fodor, C. Hoelbling, S. D. Katz, S. Krieg, and K. K. Sabzó, Phys. Lett. B 730, 99 (2014).
  • (8) S. Borsányi, Z. Fodor, J. N. Guenther, R. Kara, S. D. Katz, P. Parotto, A. Pasztor, C. Ratti, and K. K. Szabo, Phys. Rev. Lett. 125, 052001 (2020).
  • (9) K. Fukushima, Phys. Lett. B 591, 277 (2004).
  • (10) C. Ratti, M. A. Thaler, and W. Weise, Phys. Rev. D 73, 014019 (2006).
  • (11) P. Costa, M. C. Ruivo, C. A. de Sousa, and H. Hansen, Symmetry 2, 1338 (2010) .
  • (12) W. J. Fu, Z. Zhang, and Y. X. Liu, Phys. Rev. D 77, 014006 (2008).
  • (13) T. Sasaki, J. Takahashi, Y. Sakai, H. Kouno, and M. Yahiro, Phys. Rev. D 85, 056009 (2012) .
  • (14) M. Ferreira, P. Costa, and C. Providência, Phys. Rev. D 89, 036006 (2014).
  • (15) Y. Q. Zhao, S. He, D. F. Hou, L. Li, and Z. B. Li, JHEP 04, 115 (2023).
  • (16) G. Y. Shao, Z. D. Tang, X. Y. Gao, and W. B. He, Eur. Phys. J. C 78, 138 (2018).
  • (17) B. J. Schaefer, M. Wagner, and J. Wambach, Phys. Rev. D 81, 074013 (2010) .
  • (18) V. Skokov, B. Friman, and K. Redlich, Phys. Rev. C 83, 054904 (2011).
  • (19) L. M. Liu, J. Xu, and G. X. Peng, Phys. Rev. D 104, 076009 (2021).
  • (20) X. Chen, D. N. Li, D. F. Hou, and M. Huang, JHEP 2020, 73 (2020).
  • (21) M. Ferreira, P. Costa, C. Providência, Phys. Rev. D 98, 034006 (2018).
  • (22) Y. H. Yang, L. He, P. C. Chu, Nucl. Sci. Tech. 35,166 (2024).
  • (23) Y. D. Chen, D. N. Li, and M. Huang, Phys.Rev.D 106, 106002 (2022).
  • (24) F. Gao and Y. X. Liu, Nuclear Techniques 46, 040015 (2024).
  • (25) S. X. Qin, L. Chang, H. Chen, Y. X. Liu, and C. D. Roberts, Phys. Rev. Lett. 106, 172301 (2011).
  • (26) F. Gao, J. Chen, Y. X. Liu, S. X. Qin, C. D. Roberts, and S. M. Schmidt, Phys. Rev. D 93, 094019 (2016).
  • (27) F. Gao and J. M. Pawlowski, Phys. Rev. D 102, 034027 (2020).
  • (28) C. S. Fischer, J. Luecker, and C. A. Welzbacher, Phys. Rev. D 90, 034022 (2014) .
  • (29) C. Shi, Y. L. Wang, Y. Jiang, Z. F. Cui, and H. S. Zong, JHEP 1407, 014 (2014).
  • (30) W. J. Fu, J. M. Pawlowski, F. Rennecke, Phys. Rev. D 101, 054032 (2020).
  • (31) F. Rennecke and B. J. Schaefer, Phys. Rev. D 96, 016009 (2017).
  • (32) W. J. Fu, X. F. Luo, J. M. Pawlowski, F. Rennecke, R. Wen, and S. Yin, Phys. Rev. D 104, 094047 (2021)
  • (33) M. A. Stephanov, Phys. Rev. Lett. 102, 032301 (2009); Phys. Rev. Lett. 107, 052301 (2011).
  • (34) Y. G. Ma, L. G. Pang, R. Wang, K. Zhou, Chin. Phys. Lett. 40, 122101 (2023)
  • (35) M. M. Aggarwal, et al., (STAR Collaboration), Phys. Rev. Lett. 105, 022302 (2010).
  • (36) L. Adamczyk, et al., (STAR Collaboration), Phys. Rev. Lett. 112, 032302 (2014).
  • (37) J. H. Chen, et al., Nucl. Sci. Tech. 35, 214 (2024).
  • (38) X. Luo and N. Xu, Nucl. Sci. Tech. 28, 112 (2017).
  • (39) B. E. Aboona, J. Adam, L. Adamczyk, J. R. Adams, I. Aggarwal, and M. M. Aggarwal, et al., (STAR Collaboration), 130, 082301 (2023).
  • (40) Y. Zhang, D. W. Zhang, X. F. Luo, Nuclear Techniques 46, 040001 (2024).
  • (41) Q. Chen, G. L. Ma, J. H. Chen, Nuclear Techniques 46, 040013 (2023).
  • (42) C. Huang, Y. Y. Tan, R. Wen, S. Yin, and W. J. Fu, Chin. Phys. C 47, 104106 (2023).
  • (43) J. X. Shao, W. J. Fu, and Y. X. Liu, Phys. Rev. D 109, 034019 (2024).
  • (44) M. Marczenko, K. Redlich, and C. Sasaki, Phys. Rev. D 107, 054046 (2023).
  • (45) C. Liu, X. G. Deng, Y. G. Ma, Nucl. Sci. Tech. 33, 52 (2022).
  • (46) P. Chomaz, M. Colonna, and J. Randrup, Phys. Rep. 389, 263 (2004).
  • (47) J. Pochodzalla, T. Mohlenkamp, T. Rubehn, A. Schuttauf, A. Worner, E. Zude, et al., (ALADIN Collaboration), Phys. Rev. Lett. 75, 1040 (1995).
  • (48) B. Borderie, G. Tabacaru, P. Chomaz, M. Colonna, A. Guarnera, M. Parlog, et al., (NDRA Collaboration), Phys. Rev. Lett. 86, 3252 (2001).
  • (49) A. S. Botvina, I.N. Mishustin, M. Begemann-Blaich, Hubele, G. Imme, I. Iori, et al., Nucl. Phys. A584, 737 (1995).
  • (50) M. D’Agostino, A.S. Botvina, l, M. Bruno, A. Bonasera, J. R Bondorf, R. Bougault, et al., Nucl. Phys. A650, 329 (1999).
  • (51) B. K. Srivastava, R. P. Scharenberg, S. Albergo, F. Bieser, F. P. Brady, Z. Caccia, et al., (EOS Collaboration), Phys. Rev. C 65, 054617 (2002).
  • (52) J. B. Elliott, et al., (ISiS Collaboration), Phys. Rev. Lett. 88, 042701 (2002).
  • (53) W. B. He, G. Y. Shao, C. L. Xie, Phys. Rev. C 107, 014903 (2023).
  • (54) G. Y. Shao, X. Y. Gao, and W. B. He, Phys. Rev. D 101, 074029 (2020).
  • (55) K. Xu, M. Huang, arXiv:2307.12600v1.
  • (56) Y. G. Ma, Phys. Rev. Lett 83, 3617 (1999).
  • (57) X. G. Deng, P. Danielewicz, Y. G. Ma, H. Lin, Y. X. Zhang, Phys. Rev. C 105, 064613 (2022).
  • (58) M. Hempel, V. Dexheimer, S. Schramm, and I. Iosilevskiy, Phys. Rev. C 88, 014906 (2013).
  • (59) A. Mukherjee, J. Steinheimer, and S. Schramm, Phys. Rev. C 96, 025205 (2017).
  • (60) J. Xu a, L. W. Chen, C. M. Ko, B. A. Li, Y. G. Ma, Phys. Lett. B 727, 244 (2013).
  • (61) O. Savchuk, V. Vovchenko, R. V. Poberezhnyuk, M. I. Gorenstein, and H. Stoecker, Phys. Rev. C 101, 035205 (2020).
  • (62) R. Wang, Y. G. Ma, R. Wada, L. W. Chen, W. W. He, H. L. Liu, and K. J. Sun, Phys. Rev. Res. 2, 043202 (2020).
  • (63) R. V. Poberezhnyuk, V. Vovchenko, A. Motornenko, M. I. Gorenstein, and H. Stöcker, Phys. Rev. C 100, 054904 (2019).
  • (64) V. Vovchenko, M. I. Gorenstein, and H. Stöecker, Phys. Rev. Lett 118, 182301 (2017).
  • (65) R. V. Poberezhnyuk, O. Savchuk, M. I. Gorenstein, V. Vovchenko, and H. Stöecker, Phys. Rev. C 103, 024912 (2021).
  • (66) X. R. Yang and G. Y. Shao, W. B. He, Phys. Rev. C 109, 014908 (2024).
  • (67) M. Bluhm, A. Kalweit, M. Nahrgang, M. Arslandok, P. Braun-Munzinger, S. Floerchinger, Nucl. Phys. A1003 (2020) 122016.
  • (68) R. Bellwied, S. Borsányi, Z. Fodor, S. D. Katz, A. Pásztor, C. Ratti, 1 and K. K. Szabó, Phys. Rev. D 92, 114505 (2015).
  • (69) R. Wen and W. J. Fu, Chin. Phys. C 45 044112 (2021).
  • (70) H. T. Ding, S. Mukherjee, H. Ohno, P. Petreczky, and H. P. Schadler, Phys. Rev. D 92, 074043 (2015).
  • (71) S. Borsányi, Z. Fodor, J. N. Guenther, S. K. Katz, A. Pasztor, I. Portillo, C. Ratti, and K. K. Szabó, JHEP 10, 205 (2018).
  • (72) R. Bellwied, S. Borsányi, Z. Fodor, J. N. Guenther, J. Noronha-Hostler, P. Parotto, A. Pásztor, C. Ratti, and J. M. Stafford, Phys. Rev. D 101, 034506 (2020).
  • (73) W. J. Fu, Y. X. Liu, and Y. L. Wu, Phys. Rev. D 82, 074013 (2010).
  • (74) A. Bhattacharyya, P. Deb, A. Lahiri, and R. Ray, Phys. Rev. D 83, 014011 (2011).
  • (75) H. T. Ding, F. Karsch, and S. Mukherjee. Int. J. Mod. Phys. E 24, 530007 (2015).
  • (76) K. Fukushima, Phys. Rev. C 91, 044910 (2015).
  • (77) N. K. Glendenning, COMPACT STARS, Nuclear Physics, Particle Physics, and General Relativity (Springer-Verlag, New York, 1997).
  • (78) J. Cleymans, H. Oeschler, K. Redlich, and S. Wheaton, Phys. Rev. C 73, 034905 (2006).