{"title":"修正弗里德曼方程和分形黑洞热力学","authors":"S. Davood Sadatian, T. Gholame","doi":"10.1142/s0219887824501433","DOIUrl":null,"url":null,"abstract":"<p>The general relativity unification and quantum theory is a significant open problem in theoretical physics. This problem arises from the fact that these two fundamental theories, which describe gravity and the behavior of particles at the microscopic level, respectively, are currently incompatible. The unification of these theories is crucial for a complete comprehension of the fundamental forces and the nature of the universe. In this regard, the quantum properties of a Black Hole result in fundamental importance. By analyzing such properties in quantum field theory, in the first step, the gravity enters as a classical background. In semi-classical approximation, Black Holes will emit Hawking radiation with an almost thermal spectrum, while Black Hole’s entropy is proportional to the Black Hole’s horizon. Besides, Hawking’s temperature and Black Hole entropy should follow the first law of Black Hole thermodynamics. Also, Jacobson [Thermodynamics of spacetime: The Einstein equation of state, <i>Phys. Rev. Lett.</i><b>75</b> (1995) 1260, https://doi.org/10.1103/PhysRevLett.75.1260] showed shown that there is a connection between Black Hole thermodynamics and Einstein’s equation that opens the root of a potential thermodynamic nature of gravity. This issue opened a new impressive research framework in which the Einstein field equation can be expressed as a form of the first law of thermodynamics and vice versa. In this study, it is assumed that the universe has a fractal structure. Accordingly, modified Friedmann’s equations and the Black Holes thermodynamics in a fractal universe have been examined. The fractal framework shows what features and changes occur in the description of the universe, particularly in studying the thermodynamics of a Black Hole. However, the paper strategy is organized as follows: in the beginning, we consider the first thermodynamic law in a fractal universe. Then, we investigate the Friedmann equation of the fractal universe in the form of the entropy balance, this means <span><math altimg=\"eq-00001.gif\" display=\"inline\" overflow=\"scroll\"><mi>d</mi><mi>Q</mi><mo>=</mo><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub><mi>d</mi><msub><mrow><mi>S</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span>, where <span><math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"><mi>d</mi><mi>Q</mi></math></span><span></span> and <span><math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span> are the thermal energy and horizon temperature. We consider the entropy <span><math altimg=\"eq-00004.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>S</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span> have two terms; (1) obeys the usual area law and (2) the entropy production term due to the non-equilibrium thermodynamics of a fractal universe. Therefore, in a fractal universe, a term with non-equilibrium thermodynamics of spacetime may be needed. Also, we study the generalized second law of thermodynamics in a fractal universe. When the temperature of the apparent horizon and the temperature of the matter fields inside the horizon are equal, i.e. <span><math altimg=\"eq-00005.gif\" display=\"inline\" overflow=\"scroll\"><mi>T</mi><mo>=</mo><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span>, the second law of generalized thermodynamics can be obtained according to the state parameter range equation, which is consistent with the recent observations. Finally, in Sec. 6, based on the mathematical calculations, we study the various cosmological parameters such as the Hubble parameter, scale factor, deceleration parameter and equation of state parameter.</p>","PeriodicalId":50320,"journal":{"name":"International Journal of Geometric Methods in Modern Physics","volume":"26 1","pages":""},"PeriodicalIF":2.1000,"publicationDate":"2024-02-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Modified Friedmann equations and fractal Black Hole thermodynamics\",\"authors\":\"S. Davood Sadatian, T. Gholame\",\"doi\":\"10.1142/s0219887824501433\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The general relativity unification and quantum theory is a significant open problem in theoretical physics. This problem arises from the fact that these two fundamental theories, which describe gravity and the behavior of particles at the microscopic level, respectively, are currently incompatible. The unification of these theories is crucial for a complete comprehension of the fundamental forces and the nature of the universe. In this regard, the quantum properties of a Black Hole result in fundamental importance. By analyzing such properties in quantum field theory, in the first step, the gravity enters as a classical background. In semi-classical approximation, Black Holes will emit Hawking radiation with an almost thermal spectrum, while Black Hole’s entropy is proportional to the Black Hole’s horizon. Besides, Hawking’s temperature and Black Hole entropy should follow the first law of Black Hole thermodynamics. Also, Jacobson [Thermodynamics of spacetime: The Einstein equation of state, <i>Phys. Rev. Lett.</i><b>75</b> (1995) 1260, https://doi.org/10.1103/PhysRevLett.75.1260] showed shown that there is a connection between Black Hole thermodynamics and Einstein’s equation that opens the root of a potential thermodynamic nature of gravity. This issue opened a new impressive research framework in which the Einstein field equation can be expressed as a form of the first law of thermodynamics and vice versa. In this study, it is assumed that the universe has a fractal structure. Accordingly, modified Friedmann’s equations and the Black Holes thermodynamics in a fractal universe have been examined. The fractal framework shows what features and changes occur in the description of the universe, particularly in studying the thermodynamics of a Black Hole. However, the paper strategy is organized as follows: in the beginning, we consider the first thermodynamic law in a fractal universe. Then, we investigate the Friedmann equation of the fractal universe in the form of the entropy balance, this means <span><math altimg=\\\"eq-00001.gif\\\" display=\\\"inline\\\" overflow=\\\"scroll\\\"><mi>d</mi><mi>Q</mi><mo>=</mo><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub><mi>d</mi><msub><mrow><mi>S</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span>, where <span><math altimg=\\\"eq-00002.gif\\\" display=\\\"inline\\\" overflow=\\\"scroll\\\"><mi>d</mi><mi>Q</mi></math></span><span></span> and <span><math altimg=\\\"eq-00003.gif\\\" display=\\\"inline\\\" overflow=\\\"scroll\\\"><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span> are the thermal energy and horizon temperature. We consider the entropy <span><math altimg=\\\"eq-00004.gif\\\" display=\\\"inline\\\" overflow=\\\"scroll\\\"><msub><mrow><mi>S</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span> have two terms; (1) obeys the usual area law and (2) the entropy production term due to the non-equilibrium thermodynamics of a fractal universe. Therefore, in a fractal universe, a term with non-equilibrium thermodynamics of spacetime may be needed. Also, we study the generalized second law of thermodynamics in a fractal universe. When the temperature of the apparent horizon and the temperature of the matter fields inside the horizon are equal, i.e. <span><math altimg=\\\"eq-00005.gif\\\" display=\\\"inline\\\" overflow=\\\"scroll\\\"><mi>T</mi><mo>=</mo><msub><mrow><mi>T</mi></mrow><mrow><mi>h</mi></mrow></msub></math></span><span></span>, the second law of generalized thermodynamics can be obtained according to the state parameter range equation, which is consistent with the recent observations. Finally, in Sec. 6, based on the mathematical calculations, we study the various cosmological parameters such as the Hubble parameter, scale factor, deceleration parameter and equation of state parameter.</p>\",\"PeriodicalId\":50320,\"journal\":{\"name\":\"International Journal of Geometric Methods in Modern Physics\",\"volume\":\"26 1\",\"pages\":\"\"},\"PeriodicalIF\":2.1000,\"publicationDate\":\"2024-02-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"International Journal of Geometric Methods in Modern Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1142/s0219887824501433\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"PHYSICS, MATHEMATICAL\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Journal of Geometric Methods in Modern Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1142/s0219887824501433","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, MATHEMATICAL","Score":null,"Total":0}
引用次数: 0
摘要
广义相对论与量子理论的统一是理论物理学中的一个重大未决问题。这个问题源于这样一个事实,即这两个分别描述引力和微观层面粒子行为的基本理论目前互不兼容。这些理论的统一对于完全理解基本力和宇宙的本质至关重要。在这方面,黑洞的量子特性具有根本性的重要意义。通过在量子场论中分析这些特性,第一步,引力作为经典背景进入。在半经典近似中,黑洞会发出几乎是热谱的霍金辐射,而黑洞的熵与黑洞的视界成正比。此外,霍金温度和黑洞熵应该遵循黑洞热力学第一定律。另外,雅各布森 [Thermodynamics of spacetime:The Einstein equation of state, Phys. Rev. Lett.75 (1995) 1260, https://doi.org/10.1103/PhysRevLett.75.1260]表明,黑洞热力学与爱因斯坦方程之间存在着联系,从而开启了引力潜在热力学性质的根源。这个问题开启了一个新的令人印象深刻的研究框架,其中爱因斯坦场方程可以表达为热力学第一定律的一种形式,反之亦然。在这项研究中,假设宇宙具有分形结构。因此,对分形宇宙中的修正弗里德曼方程和黑洞热力学进行了研究。分形框架显示了宇宙描述中出现的特征和变化,特别是在研究黑洞热力学时。不过,本文的策略安排如下:首先,我们考虑分形宇宙中的第一热力学定律。然后,我们以熵平衡的形式研究分形宇宙的弗里德曼方程,即 dQ=ThdSh,其中 dQ 和 Th 分别为热能和地平线温度。我们认为熵 Sh 有两个项:(1)服从通常的面积定律;(2)由于分形宇宙的非平衡热力学而产生的熵项。因此,在分形宇宙中,可能需要一个时空非平衡热力学项。此外,我们还研究了分形宇宙中的广义热力学第二定律。当视界温度和视界内物质场温度相等时,即T=Th,根据状态参数范围方程可以得到广义热力学第二定律,这与最近的观测结果是一致的。最后,在第 6 节中,基于数学计算,我们研究了各种宇宙学参数,如哈勃参数、尺度因子、减速参数和状态方程参数。
Modified Friedmann equations and fractal Black Hole thermodynamics
The general relativity unification and quantum theory is a significant open problem in theoretical physics. This problem arises from the fact that these two fundamental theories, which describe gravity and the behavior of particles at the microscopic level, respectively, are currently incompatible. The unification of these theories is crucial for a complete comprehension of the fundamental forces and the nature of the universe. In this regard, the quantum properties of a Black Hole result in fundamental importance. By analyzing such properties in quantum field theory, in the first step, the gravity enters as a classical background. In semi-classical approximation, Black Holes will emit Hawking radiation with an almost thermal spectrum, while Black Hole’s entropy is proportional to the Black Hole’s horizon. Besides, Hawking’s temperature and Black Hole entropy should follow the first law of Black Hole thermodynamics. Also, Jacobson [Thermodynamics of spacetime: The Einstein equation of state, Phys. Rev. Lett.75 (1995) 1260, https://doi.org/10.1103/PhysRevLett.75.1260] showed shown that there is a connection between Black Hole thermodynamics and Einstein’s equation that opens the root of a potential thermodynamic nature of gravity. This issue opened a new impressive research framework in which the Einstein field equation can be expressed as a form of the first law of thermodynamics and vice versa. In this study, it is assumed that the universe has a fractal structure. Accordingly, modified Friedmann’s equations and the Black Holes thermodynamics in a fractal universe have been examined. The fractal framework shows what features and changes occur in the description of the universe, particularly in studying the thermodynamics of a Black Hole. However, the paper strategy is organized as follows: in the beginning, we consider the first thermodynamic law in a fractal universe. Then, we investigate the Friedmann equation of the fractal universe in the form of the entropy balance, this means , where and are the thermal energy and horizon temperature. We consider the entropy have two terms; (1) obeys the usual area law and (2) the entropy production term due to the non-equilibrium thermodynamics of a fractal universe. Therefore, in a fractal universe, a term with non-equilibrium thermodynamics of spacetime may be needed. Also, we study the generalized second law of thermodynamics in a fractal universe. When the temperature of the apparent horizon and the temperature of the matter fields inside the horizon are equal, i.e. , the second law of generalized thermodynamics can be obtained according to the state parameter range equation, which is consistent with the recent observations. Finally, in Sec. 6, based on the mathematical calculations, we study the various cosmological parameters such as the Hubble parameter, scale factor, deceleration parameter and equation of state parameter.
期刊介绍:
This journal publishes short communications, research and review articles devoted to all applications of geometric methods (including commutative and non-commutative Differential Geometry, Riemannian Geometry, Finsler Geometry, Complex Geometry, Lie Groups and Lie Algebras, Bundle Theory, Homology an Cohomology, Algebraic Geometry, Global Analysis, Category Theory, Operator Algebra and Topology) in all fields of Mathematical and Theoretical Physics, including in particular: Classical Mechanics (Lagrangian, Hamiltonian, Poisson formulations); Quantum Mechanics (also semi-classical approximations); Hamiltonian Systems of ODE''s and PDE''s and Integrability; Variational Structures of Physics and Conservation Laws; Thermodynamics of Systems and Continua (also Quantum Thermodynamics and Statistical Physics); General Relativity and other Geometric Theories of Gravitation; geometric models for Particle Physics; Supergravity and Supersymmetric Field Theories; Classical and Quantum Field Theory (also quantization over curved backgrounds); Gauge Theories; Topological Field Theories; Strings, Branes and Extended Objects Theory; Holography; Quantum Gravity, Loop Quantum Gravity and Quantum Cosmology; applications of Quantum Groups; Quantum Computation; Control Theory; Geometry of Chaos.