Hanwen Feng, Yuchen Huang,, Wei Hong,, Jun Tao,∗Center for Theoretical Physics, College of Physics, Sichuan University, Chengdu, 610064, China
First author contact: Author to whom any correspondence should be addressed. Received:2020-12-22Revised:2021-01-29Accepted:2021-02-8Online:2021-03-04
Abstract We investigate the thermodynamical properties of charged torus-like black holes and take it as the working substance to study the heat engines. In the extended phase space, by interpreting the cosmological constant as the thermodynamic pressure, we derive the thermodynamical quantities by the first law of black hole thermodynamics and obtain the equation of state. Then, we calculate the efficiency of the heat engine in the Carnot cycle as well as the rectangular cycle, and investigate how the efficiency changes with respect to volume. In addition, to avoid a negative temperature, we emphasize that the charge of this black hole cannot be arbitrary. Last, we check the calculation accuracy of a benchmark scheme and discuss the upper bound and lower bound for charged torus-like black hole in the scheme. Keywords：charged torus-like black holes;heat engines;benchmark scheme
PDF (545KB)MetadataMetricsRelated articlesExportEndNote|Ris|BibtexFavorite Cite this article Hanwen Feng, Yuchen Huang, Wei Hong, Jun Tao. Charged torus-like black holes as heat engines. Communications in Theoretical Physics, 2021, 73(4): 045403- doi:10.1088/1572-9494/abe3ef
1. Introduction
The pioneering work of Hawking and Bekenstein [1–4] stimulates the interest in the study of black hole thermodynamics. Hawking temperature and Bekenstein–Hawking entropy provides a profound insight into the nature of quantum gravity. In the extended framework, the cosmological constant is considered as a dynamical parameter and the mass of an Anti-de Sitter (AdS) black hole can be interpreted as the enthalpy of the space [5, 6]. Compared with the classical thermodynamic, people have gradually established four laws of black hole thermodynamics.
The holographic principle is developed from the Bekenstein–Hawking entropy, while the thermodynamic behaviour of black holes in AdS space reveals the strong coupling gauge theory through various proposed dualities [7]. Based on this assumption, Johnson proposed a heat engine defined in the extended thermodynamical space, which takes the AdS black holes as the working substance [8]. For a negative cosmological constant, the engine cycle corresponds to a process defined on the space of dual field theories. To understand the holographic heat engine, it is rather important to investigate the microscopic structure. Many different theories have been studied to explore the microscopic property of black holes [9–14]. For further investigation, a concept, i.e. the number density n of the virtual black hole molecules, is introduced to study the behaviours of the microscopic thermodynamic variables [15, 16]. It can be regarded as the order parameter to measure the microscopic degrees of freedom and it is related to the size or radius of the black hole [17]. From this point, we can take the process of a black hole doing work as the changes in n, but it remains a conception and still requires more effort to understand the microscopic structure.
The heat engine is defined in the P–V space as a closed path. At first, we can calculate the efficiency of the holographic heat engines of black holes with vanishing specific heat at constant volume (CV = 0) in analytical way. Next, Johnson investigated the efficiency of Born–Infeld black hole in the rectangular cycle [18] and then obtained a efficiency formula for heat engines in this rectangular cycle [19, 20]. When the engine is defined as a rectangular cycle expressed with mass and internal energy of the black hole, the calculation for black holes with CV ≠ 0 is capable as well [21]. Since various black holes can be the working substance of a heat engine, and the efficiency is a dimensionless quantity, we can compare different black holes’ efficiency and investigate their thermodynamical properties further. To avoid the case where one particular heat engine yields advantages for one specific black hole, Chakraborty and Johnson proposed the benchmarking scheme [22, 23], which separates a complicated cycle into rectangular cycles and calculates the efficiency approximately with numerical method. Recently, black holes in massive gravity have been discussed as heat engines in [24–26]. Then, researchers have studied the thermodynamics and heat engine efficiency of charged accelerating AdS black holes [27, 28], nonlinear black holes [29, 30] and the general class of accelerating, rotating and charged Plebanski–Demianski black holes [30]. Moreover, Johnson have investigated the de sitter Black holes in [32]. More work on heat engines can be found in [33–43].
In this paper, we investigate the heat engine efficiency of the torus-like black hole in Carnot cycle, rectangular cycle and the benchmark cycle. The torus-like black hole is a static solution of the Einstein-Maxwell equation, whose event horizon has ${S}_{1}\times {S}_{1}\times {\mathbb{R}}$ topology [44–48]. Each surface of this black hole of the spacetime at constant radius has a toroidal topology which is different from that of the asymptotically flat spacetimes.
This paper is organized as follows. In section 2, we investigate the thermodynamic property of a torus-like black hole and derive the expression for thermodynamic quantities. In section 3, we construct a rectangular heat engine cycle, and then take the torus-like black hole as the working substance to study its efficiency with respect to volume. Since the Carnot heat engine is theoretically with the maximum efficiency, we compare it with the rectangular engine to check. In section 4, we calculate the efficiency of benchmark cycle and investigate how the upper bound limits the charge. In the end, the conclusion is given in section 5.
2. Thermodynamics of charged torus-like black hole
We are interested in charged torus-like black hole, the ansatz for metric can be written as [44],$\begin{eqnarray}{\rm{d}}{s}^{2}=-f(r){\rm{d}}{t}^{2}+\displaystyle \frac{{\rm{d}}{r}^{2}}{f(r)}+{r}^{2}({\rm{d}}{\theta }^{2}+{\rm{d}}{\psi }^{2}),\end{eqnarray}$with$\begin{eqnarray}f(r)=-\displaystyle \frac{{\rm{\Lambda }}{r}^{2}}{3}-\displaystyle \frac{2M}{\pi r}+\displaystyle \frac{4{Q}^{2}}{\pi {r}^{2}},\end{eqnarray}$where M and Q are mass and electric charge of the black hole, Λ is the cosmological constant. The black hole mass can be obtained by f(r+) = 0, where r+ is the event horizon radius,$\begin{eqnarray}M=\displaystyle \frac{12{Q}^{2}-\pi {r}_{+}^{4}{\rm{\Lambda }}}{6{r}_{+}}.\end{eqnarray}$In 4D AdS spacetime, the negative cosmological constant can be considered as thermodynamical pressure with $P=-\tfrac{{\rm{\Lambda }}}{8\pi }$ [5], so that M can be rewritten as$\begin{eqnarray}M=\displaystyle \frac{6{Q}^{2}+4P{\pi }^{2}{r}_{+}^{4}}{3{r}_{+}}.\end{eqnarray}$The variation of the mass takes on the form$\begin{eqnarray}{\rm{d}}M=-\displaystyle \frac{2{Q}^{2}-4P{\pi }^{2}{r}_{+}^{4}}{{r}_{+}^{2}}{\rm{d}}{r}_{+}+\displaystyle \frac{4Q}{{r}_{+}}{\rm{d}}Q+\displaystyle \frac{4{\pi }^{2}{r}_{+}^{3}}{3}{\rm{d}}P.\end{eqnarray}$
According to the definition of surface gravity, the Hawking temperature is only related to the black hole metric [48],$\begin{eqnarray}T=\displaystyle \frac{f^{\prime} ({r}_{+})}{4\pi }=\displaystyle \frac{-12{Q}^{2}+3{{Mr}}_{+}+8P{\pi }^{2}{r}_{+}^{4}}{6{\pi }^{2}{r}_{+}^{3}}.\end{eqnarray}$Substituting equation (4) into (6), the temperature can be written as$\begin{eqnarray}T=-\displaystyle \frac{{Q}^{2}-2{P}^{2}{r}_{+}^{4}}{{\pi }^{2}{r}_{+}^{3}}.\end{eqnarray}$With the relation between the Bekenstein–Hawking entropy and the surface area of the event horizon, the entropy of this black hole can be expressed as$\begin{eqnarray}S={\pi }^{2}{r}_{+}^{2}.\end{eqnarray}$The thermodynamic volume and electric potential at the event horizon are given by$\begin{eqnarray}V={\left(\displaystyle \frac{\partial M}{\partial P}\right)}_{S,Q}=\displaystyle \frac{4{\pi }^{2}{r}_{+}^{3}}{3},\ {\rm{\Phi }}={\left(\displaystyle \frac{\partial M}{\partial Q}\right)}_{P,S}=\displaystyle \frac{4Q}{{r}_{+}}.\end{eqnarray}$In the extended thermodynamics, the mass of an AdS black hole is interpreted to the enthalpy of spacetime [5]. And equations (5)–(9) shows the first law of thermodynamics is satisfied,$\begin{eqnarray}{\rm{d}}M=T{\rm{d}}S+{\rm{\Phi }}{\rm{d}}Q+V{\rm{d}}P.\end{eqnarray}$
As the entropy and volume are both the function of black holes horizon, the heat capacity at constant volume vanishes,$\begin{eqnarray}{C}_{V}=T{\left(\displaystyle \frac{\partial S}{\partial T}\right)}_{V}=0.\end{eqnarray}$The state equation of the black hole can be derived from equations (7) and (9),$\begin{eqnarray}P=\displaystyle \frac{{\pi }^{2/3}}{3\sqrt[3]{6}}\left(\displaystyle \frac{4{Q}^{2}}{{V}^{4/3}}+\displaystyle \frac{3T}{{V}^{1/3}}\right).\end{eqnarray}$As the critical point satisfies the condition that the first-order partial derivative with respect to volume of pressure and the second-order partial derivative are 0, we derive these two partial derivatives to find this point$\begin{eqnarray}\displaystyle \frac{\partial P}{\partial V}=-\displaystyle \frac{{\pi }^{2/3}\left(16{Q}^{2}+3{TV}\right)}{9\sqrt[3]{6}{V}^{7/3}}.\end{eqnarray}$From equation (13), we can see that $\tfrac{\partial P}{\partial V}=0$ is not feasible as the square term, temperature and volume are always positive. This result indicates the absence of critical point as shown in figure 1, and correspondingly, this black hole has no second-order phase transition [49].
For the purpose of studying the behaviour of torus-like black hole as a heat engine, we prefer writing the enthalpy M entirely in terms of P and V by substituting equation (9) into (4), and then the expression yields:$\begin{eqnarray}M={PV}+2{Q}^{2}\sqrt[3]{\displaystyle \frac{4{\pi }^{2}}{3V}}.\end{eqnarray}$
It should be noted that, when the torus-like black hole carries no electric charge, i.e. Q = 0, its enthalpy M reduces to the same form as that of ideal gas, namely M = PV [22], which will be discussed later.
3. Charged torus-like black hole as a heat engine
Since the equation of state for the charged black hole is obtained, we could discuss further by considering this black hole as a heat engine and calculating its efficiency. In the following sections, the black hole is set in thermodynamical cycles and produces work via the PdV term. We denote the heat absorbed as QH, and the heat exhausted as QC, so that the mechanical work is W = QH − QC. The efficiency is the ratio of mechanical work W to heat absorbed QH [24],$\begin{eqnarray}\eta =\displaystyle \frac{W}{{Q}_{H}}=1-\displaystyle \frac{{Q}_{C}}{{Q}_{H}}.\end{eqnarray}$The Carnot cycle consists of two isothermal paths and two adiabatic paths and has the highest efficiency. Note that for the black hole engine, the entropy remains constant if the volume does not change, so the adiabatic path is equivalent to the isochoric path. Moreover, we define a rectangular cycle with two isochoric and two isobaric paths and compare its efficiency with that of Carnot cycle. We compare the diagram of the two cycles in figure 2.
Figure 1.
New window|Download| PPT slide Figure 1.The figure shows P versus V for different temperature. Here Q is fixed at 1.
The Carnot heat engine is between two different temperatures, we define the higher temperature as TH and the lower one as TL, which are connected through the isochoric paths. We can know from figure 2 that TH = T1 = T2, TL = T3 = T4, V1 = V4 and V2 = V3 for Carnot cycle. The heat QH and QC can be calculated in the process of isothermal expansion and compression [24],$\begin{eqnarray}{Q}_{H}={T}_{H}{\rm{\Delta }}{S}_{1\to 2}={T}_{H}\displaystyle \frac{{\left(3\pi \right)}^{2/3}}{2\times {2}^{1/3}}\left({V}_{2}^{2/3}-{V}_{1}^{2/3}\right),\end{eqnarray}$$\begin{eqnarray}{Q}_{C}={T}_{L}{\rm{\Delta }}{S}_{3\to 4}={T}_{L}\displaystyle \frac{{\left(3\pi \right)}^{2/3}}{2\times {2}^{1/3}}\left({V}_{3}^{2/3}-{V}_{4}^{2/3}\right).\end{eqnarray}$Since the volume is connected through isochoric paths, the expression for heat engine efficiency in equation (15) can be written as:$\begin{eqnarray}{\eta }_{c}=1-\displaystyle \frac{{Q}_{C}}{{Q}_{H}}=1-\displaystyle \frac{{T}_{L}}{{T}_{H}}.\end{eqnarray}$In order to investigate the relationship between efficiency and volume, one can substitute equations (3) and (9) into (6), the temperature could be rewritten as,$\begin{eqnarray}T(P,V,Q)=\displaystyle \frac{3\sqrt[3]{6}{{PV}}^{4/3}-4{\pi }^{2/3}{Q}^{2}}{3{\pi }^{2/3}V}.\end{eqnarray}$Then we can obtain the efficiency of Carnot engine,$\begin{eqnarray}{\eta }_{c}=1-\displaystyle \frac{{V}_{2}\left(3\sqrt[3]{6}{P}_{4}{V}_{4}^{4/3}-4{\pi }^{2/3}{Q}^{2}\right)}{{V}_{4}\left(3\sqrt[3]{6}{P}_{2}{V}_{2}^{4/3}-4{\pi }^{2/3}{Q}^{2}\right)}.\end{eqnarray}$
Using the above formula to compute Carnot heat engine efficiency with the volume of this black hole is straightforward. Here we choose parameters P2 = 4, P4 = 1 and V2 = 4, V4 = 1, with different charge Q. Then we can plot the efficiency of Carnot cycle versus the black hole volume V2 in figure 3. It shows the efficiency increases monotonously and flattens out with the increase of volume. Note that for a larger volume, the corresponding efficiency is higher.
Figure 3.
New window|Download| PPT slide Figure 3.The heat engine efficiency of Carnot cycle versus the black hole volume V2 for different charge Q, where we set V4 = 1, P2 = 4, and P4 = 1.
It should be noted that the temperature cannot be negative, otherwise it makes no sense in physics, so that the charge Q is not arbitrary. Considering the extremal black hole situation T = 0, the maximum charge reads,$\begin{eqnarray}{Q}^{2}\leqslant \displaystyle \frac{3\sqrt[3]{6}{{PV}}^{4/3}}{4{\pi }^{2/3}}.\end{eqnarray}$We can set P1 = P2 = 4, P3 = P4 = 1, V1 = V4 = 1, and V2 = V3 = 4, after taking both the lower temperature and the higher one into account, the charge of black hole is restricted as −0.797 ≲ Q ≲ 0.797 to make the expression physical. We can plot the efficiency changing with the varying charge in figure 4. There are two cut-off points ${Q}_{{c}_{1}}=0.797$ and ${Q}_{{c}_{2}}=-0.797$ in the curve, when charge Q reaches the limitation, the black hole temperature T = 0 and the heat engine efficiency η = 1. The cut-off point here reveals the information of Hawking temperature and corresponds to the extremal black holes. Besides, it can be seen from the figure 4 that the efficiency of the Carnot heat engine has a minimum value, if the torus-like black hole carries no electric charge.
As we will see, the rectangular cycle is the most natural cycle to consider for all AdS black holes, because it can be generalized to an algorithm, which allows more complex cycles to be numerically calculated. The rectangular cycle goes through isobaric and isochoric paths, although there are four states in the cycle, we can set P1 = P2, P3 = P4, V1 = V4, V2 = V3 as shown in figure 2. The heat engine efficiency for the rectangle cycle can be calculated by a formula deduced in [19, 20],$\begin{eqnarray}\eta =1-\displaystyle \frac{{M}_{3}-{M}_{4}}{{M}_{2}-{M}_{1}}=\displaystyle \frac{3\left({P}_{2}-{P}_{4}\right)}{3{P}_{2}-2{(6\pi )}^{2/3}{Q}^{2}/\alpha },\end{eqnarray}$where$\begin{eqnarray}\alpha ={V}_{4}{V}_{2}^{1/3}+{V}_{4}^{2/3}{V}_{2}^{2/3}+{V}_{4}^{1/3}{V}_{2}.\end{eqnarray}$
According to equation (22), we can choose parameters P1 = P2 = 4, P4 = 1 and V1 = V4 = 1, and then we plot the heat engine efficiency of rectangle cycle with respect to the volume V2 with different charge Q in figure 5. It is obvious that when the charge is fixed, the efficiency curve flattens out as the volume increases and tends to a stable value. Meanwhile, the larger volume V2 leads to a lower efficiency, which differs from the situation for the Carnot cycle we mentioned above. On the other hand, for the same volume, the larger Q results in higher efficiency both for Carnot cycle and rectangular cycle.
Figure 5.
New window|Download| PPT slide Figure 5.The engine efficiency of rectangle cycle versus the black hole volume V2, with parameters set same as the Carnot cycle.
4. The benchmark cycle for charged torus-like black hole
In this section, we introduce a benchmark cycle [22], which could be parameterised as a circle. The scheme is adequately complicated as the thermodynamic variables changes on every segment of the cycle, and thus it is more general than regular cycles. This research method can be applied to compare the heat engine efficiency of different black holes. In addition, an upper bound is obtained in [21] which indicates the efficiency of this cycle is always lower than a specific value.
Generally, the heat engine efficiency is calculated by numerical method. To simplify our calculation, we choose a circular cycle with center of which set as (Po, Vo) and radius as R. We overlay our circular cycle onto the N × N regular lattice of squares, and we require N to be even for simplicity. The side length of every square is 2L/N, which ensures those squares can cover the circle. Next we check the cases where two squares share a common isobar and it intersects the circle. Then we calculate the ΔM of the left and right endpoints of the isobar.
The heat input QH will be the sum of ΔM in the upper semicircle and the heat output QC is given by the sum of ΔM in the lower semicircle. Thus we can calculate the efficiency with the numerical method [22]$\begin{eqnarray}\eta =1-\displaystyle \frac{{Q}_{C}}{{Q}_{H}},\end{eqnarray}$where,$\begin{eqnarray}\begin{array}{rcl}{Q}_{H} & = & \displaystyle \sum _{i}({M}_{2}^{i}-{M}_{1}^{i}),\\ {Q}_{C} & = & \displaystyle \sum _{j}({M}_{3}^{j}-{M}_{4}^{j}).\end{array}\end{eqnarray}$The result converges to the right value with a larger N, as it makes the square smaller and thus fit to the circle more perfectly. Figure 6 shows that as N increases, the efficiency approaches to an exact result.
Figure 6.
New window|Download| PPT slide Figure 6.Efficiency of the charged torus-like black hole calculated with the numerical method. Here we set the circle origin at Vo = 110 and Po = 20, the charge Q = 20.0 and radius R = 10.0. The efficiency equals to 0.587 226 when N = 500.
In a particular case where the specific heat capacity at constant volume CV = 0, we can calculate the efficiency in an analytical way. Then we can check the the accuracy of the above numerical method by comparing it with an analytical method. The heat engine efficiency would be [21]$\begin{eqnarray}\eta =\displaystyle \frac{2\pi }{\pi +\tfrac{2{\rm{\Delta }}M}{{R}^{2}}},\end{eqnarray}$where ΔM is the enthalpy difference of two points at the left and right ends of the circle,$\begin{eqnarray}{\rm{\Delta }}M=M({V}_{{\rm{o}}}+R,{P}_{{\rm{o}}})-M({V}_{{\rm{o}}}-R,{P}_{{\rm{o}}}).\end{eqnarray}$By substituting those parameters of figure 6 into equation (26), we obtain the analytical result ηa = 0.589 322. Comparing with the results of numerical method when N reaches 500, ηn = 0.587 226, we can conclude that the error of the numerical method is within the acceptable range and the scheme can be applied to the case where analytical method does not work.
In the benchmark scheme, an upper bound for the efficiency of black holes with CV = 0 in circular cycles with the narrow cycle limit and low temperature limit is obtained [21],$\begin{eqnarray}\eta \leqslant \displaystyle \frac{2\pi }{\pi +4}.\end{eqnarray}$It is independent of both theory and spacetime dimension, with equality obtained for extremal black holes in the small cycle limit.
As we mentioned earlier, when the black hole charge Q = 0, its enthalpy M is the same as that of ideal gas [22], and we can get the lower limit of the efficiency of the torus-like black hole heat engine. The efficiency of ideal gas is independent of V and spacetime and only depends on the pressure at the center of the cycle and the radius of the circle, as mentioned in [18, 22, 23]$\begin{eqnarray}\eta =\displaystyle \frac{2\pi }{\pi +4P/R}.\end{eqnarray}$
We conclude the consideration of benchmarking of the black hole heat engines, and present it in figure 7. The efficiency of ideal gas model is 0.5639 at P = 20.0 and R = 10.0. When Q = 57.7431, η reaches the extremal limit 0.8798. As equation (14) shows, the mass of torus-like black hole has the same form as the ideal gas when the black hole carries no charge, so the efficiency curve of the black hole and the ideal gas start at the exact point. On the other hand, the top horizontal line is the extremal limit, and it forbids the efficiency to exceed itself.
Figure 7.
New window|Download| PPT slide Figure 7.This figure plots the efficiency of two black holes with respect to Q in the benchmark cycle.
5. Conclusion
In this paper, we have studied the thermodynamical behaviour of charged torus-like black hole in the extended phase space. By considering the cosmological constant in AdS space as the thermodynamical pressure and the mass as the enthalpy in the first law of thermodynamics, we can obtain all the thermodynamical quantities and the relationship between them. We derive the equation of state with thermodynamical quantities and find there does not exist a critical point in the phase diagram which represents the absence of phase transition.
Then, we considered charged torus-like black hole as a working substance and studied the holographic heat engine by Carnot cycle and rectangular cycle. The Carnot cycle consists of two isothermal paths and two adiabatic paths, it is always theoretically highest according to the second law of thermodynamics, and thus it provides an upper bound for us to check the calculation. The rectangular cycle is made up of two isochoric paths and two isobaric paths. It works for all black holes, not requiring the specific heat capacity CV = 0, and it could be an operation unit in other cycles and enable us to calculate the efficiency of the benchmark cycle with numerical methods. From figures 5 and 3, we conclude that the rectangular efficiency decreases monotonously with respect to the difference between the volume at initial and final states, while the Carnot efficiency does the opposite.
The heat engine cycle in the benchmark scheme is more complicated, and we differentiate the curve into line segments and calculate the efficiency approximately. We compare the numerical result with the analytical result and check the calculation accuracy of numerical methods, then we find the error is acceptable. Due to the fact that the torus-like black hole has the same enthalpy with the ideal gas when Q = 0 and that Q increases the efficiency, the efficiency of ideal gas is a lower bound for the torus-like black hole. On the other hand, the efficiency of a certain class of asymptotically AdS black holes with CV in the circular cannot exceed a upper bound as well.
Acknowledgments
We are grateful to thank Peng Wang and Feiyu Yao for useful discussions. This work is supported by NSFC (Grant No.11947408).
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,, Wei Hong
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