| Literature DB >> 33286771 |
Yu-Han Ma1,2.
Abstract
Heat engines used to output useful work have important practical significance, which, in general, operate between heat baths of infinite size and constant temperature. In this paper, we study the efficiency of a heat engine operating between two finite-size heat sources with initial temperature difference. The total output work of such heat engine is limited due to the finite heat capacity of the sources. We firstly investigate the effects of different heat capacity characteristics of the sources on the heat engine's efficiency at maximum work (EMW) in the quasi-static limit. Moreover, it is found that the efficiency of the engine operating in finite-time with maximum power of each cycle is achieved follows a simple universality as η=ηC/4+OηC2, where ηC is the Carnot efficiency determined by the initial temperature of the sources. Remarkably, when the heat capacity of the heat source is negative, such as the black holes, we show that the heat engine efficiency during the operation can surpass the Carnot efficiency determined by the initial temperature of the heat sources. It is further argued that the heat engine between two black holes with vanishing initial temperature difference can be driven by the energy fluctuation. The corresponding EMW is proved to be ηMW=2-2.Entities:
Keywords: efficiency at maximum power; efficiency at maximum work; finite-size heat source
Year: 2020 PMID: 33286771 PMCID: PMC7597076 DOI: 10.3390/e22091002
Source DB: PubMed Journal: Entropy (Basel) ISSN: 1099-4300 Impact factor: 2.524
Bound for efficiency in different case. Here t is the operation time of the heat engine and C is the heat capacity of the heat source. In the case engine working in quasi-static cycle between infinite heat bath, i.e., , , the maximum achievable efficiency, as stated by Carnot, is the Carnot efficiency . For the engine operates in finite time, i.e., , , Esposito et al. [41] give the bounds for the efficiency at maximum power (EMP), , with low-dissipation Carnot-like engine. The bounds for efficiency at maximum work (EMW) (, ), , and efficiency at maximum power for each cycle (, ), , are obtained in this paper. The detailed derivations are illustrated in Section 2.1 and Section 3, respectively. The bounds in the latter two cases for and in this table are limited to the heat source having a positive and constant heat capacity. The bounds correspond to heat capacity change with temperature are discussed in Section 2.2 while the negative heat capacity case are discussed in Section 4.
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Figure 1Heat engine working between two finite-size heat sources. () and () are the temperature and heat capacity of the high (low) temperature source (), respectively. is the output work of the engine per cycle while is the heat absorbed from the hot source and the heat releases to the cold source.
Figure 2EMW as the function of with different The curves relate to infinite heat capacity (in comparison with the hot one) of low-temperature source () and infinite heat capacity (in comparison with the cold one) of high-temperature source () are given by Equation (13). The other are plot with Equation (12).
Figure 3EMW as the function of with different source dimension n. The curves relate to and are given by Equation (19) and Equation (20), respectively.
Figure 4EMW as the function of with different for source dimension . The curves with finite are plotted with Equation (17), while the curves relate to and are given by Equation (19) and Equation (20), respectively.
Figure 5Upper () and lower () bounds for efficiency of the heat engine in finite-time operation as the function of in different limit of . and respectively correspond to and . Here and respectively characterize the asymmetry in size and in dissipation of the two heat sources. As the comparison, the red(black) dashed line represent the upper (lower) bound of EMP in the reversible limit given by Equation (13). Other are plotted with Equations (38)–(41).
Figure 6Efficiency at maximum work of a heat engine working between two Schwarzschild black holes.