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On Stochastic Pure-Cubic Optical Soliton Solutions of Nonlinear Schrödinger Equation Having Power Law of Self-Phase Modulation 论具有自相调制幂律的非线性薛定谔方程的随机纯立方体光学孤子解
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-29 DOI: 10.1007/s10773-024-05756-y
Aydin Secer, Ismail Onder, Handenur Esen, Neslihan Ozdemir, Melih Cinar, Hasan Cakicioglu, Selvi Durmus, Muslum Ozisik, Mustafa Bayram

In this study, we focus on the stochastic pure-cubic optical solitons of the nonlinear Schrödinger equation, characterized by a parabolic law of nonlinearity. The nonlinear Schrödinger equation models are crucial for simulating pulse propagation in optical fibers especially ultrashort pulses. To obtain optical soliton solutions, we employ the effective and well-known the new Kudryashov and the generalized Kudryashov methods. Through these methods, we successfully derive dark, bright, and singular optical soliton solutions. Our findings are illustrated with 2D and 3D graphics for clarity. A significant aspect of our study is the inclusion of stochasticity in the model. We specifically examine the impact of white noise on the solutions. This effect is detailed in the results section, with corresponding graphs. Throughout our research, we did not encounter any restrictive factors that hindered access to the results. Ultimately, considering the growing number of studies on optical fibers, our work stands out by being the first to obtain optical solutions for this specific model and by investigating the influence of stochastic theories on wave behavior.

在本研究中,我们重点研究非线性薛定谔方程的随机纯立方光孤子,其特点是非线性抛物线规律。非线性薛定谔方程模型对于模拟光纤中的脉冲传播,尤其是超短脉冲传播至关重要。为了获得光学孤子解,我们采用了有效的、众所周知的新库德里亚绍夫方法和广义库德里亚绍夫方法。通过这些方法,我们成功地推导出了暗光、亮光和奇异光孤子解。我们用二维和三维图形对研究结果进行了清晰的说明。我们研究的一个重要方面是在模型中加入了随机性。我们特别研究了白噪声对解法的影响。结果部分详细介绍了这种影响,并配有相应的图表。在整个研究过程中,我们没有遇到任何妨碍获取结果的限制性因素。最后,考虑到有关光纤的研究越来越多,我们的研究工作通过首次获得这一特定模型的光学解以及研究随机理论对波行为的影响而脱颖而出。
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引用次数: 0
Impact of Radial Perturbations on Expansion-free Anisotropic Fluid Spheres in D-dimensional Modified Gravity 径向扰动对 D 维修正重力中无膨胀各向异性流体球的影响
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-29 DOI: 10.1007/s10773-024-05757-x
Bander Almutairi, M. Z. Bhatti, M. Yousaf, Z. Yousaf, A. S. Khan

In this manuscript, we have continued the work of Herrera et al. (Gen. Relativ. Gravit. 44, 1143, 2012) to investigate the instability of non-static spheres supported by anisotropic matter configuration in the background of D-dimensional Einstein gravity. For this purpose, we assume that our relativistic sphere undergoes adiabatic evolution with a vanishing expansion scalar condition. We compute gravitational field equations, conservation equations, and junction conditions in D-dimensional Einstein theory. After considering the evolution of the systems under an expansion-free background, some significant constraints are established by using a perturbation scheme. This leads us to develop the dynamical instability of expansion-free anisotropic fluid spheres in the Newtonian (N) and Post-Newtonian (PN) domains. After focusing on the N and PN eras, our study reveals that the adiabatic index ((Gamma )), does not contribute to the instability ranges in these domains. Instead, these ranges are being determined solely by the anisotropy of fluid pressure, D-dimensional Einstein gravity parameter, and the radial energy density profile.

在本手稿中,我们延续了埃雷拉等人(Gen. Relativ. Gravit. 44, 1143, 2012)的工作,研究了在 D 维爱因斯坦引力背景下由各向异性物质配置支撑的非静态球体的不稳定性。为此,我们假设相对论球体在膨胀标量条件消失的情况下经历绝热演化。我们计算了 D 维爱因斯坦理论中的引力场方程、守恒方程和交界条件。在考虑了系统在无膨胀背景下的演化之后,我们使用扰动方案建立了一些重要的约束条件。由此,我们发展了牛顿(N)和后牛顿(PN)域中无膨胀各向异性流体球的动力学不稳定性。在聚焦于 N 和 PN 时代之后,我们的研究揭示出绝热指数((Gamma ))对这些域中的不稳定性范围没有贡献。相反,这些范围完全是由流体压力各向异性、D维爱因斯坦引力参数和径向能量密度剖面决定的。
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引用次数: 0
Dynamics of Bifurcation, Chaos, Sensitivity and Diverse Soliton Solution to the Drinfeld-Sokolov-Wilson Equations Arise in Mathematical Physics 数学物理学中出现的德林费尔德-索科洛夫-威尔逊方程的分岔、混沌、敏感性和多样孤子解的动力学问题
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-29 DOI: 10.1007/s10773-024-05759-9
Laila A. AL-Essa, Mati ur Rahman

In this study, we present an amalgamation of solitary wave solutions for the fractional coupled Drinfeld-Sokolov-Wilson (FCDSW) equations, a versatile mathematical model with significant applications in fluid dynamics, plasma physics, and nonlinear dynamics. By leveraging the two recently developed computational approaches, namely the modified Sardar sub-equation (MSSE) method and the improved (mathbb {F})- expansion method, we manifested the novel soliton solutions in the form of dark, dark-bright, bright-dark, singular, periodic, exponential, and rational forms. Furthermore, we also extracted W-shape, V-shape, mixed trigonometric, and hyperbolic soliton wave solutions, which are not reported in previously. Also, the modulation instability (MI) of the proposed model is also examined. To further understand the dynamics of the FCDSW equations, we conducted a detailed bifurcation analysis to investigate the bifurcation events exhibited by these equations. A sensitivity analysis was also performed to assess the model’s robustness against variations in initial conditions and parameters, offering valuable insights into the system’s susceptibility to perturbations. We proved the effectiveness of our suggested techniques in the analysis of the FCDSW equations using analytical tools and numerical simulations. Our results provide new insights into the behavior and solutions of the FCDSW equations and enhance the mathematical tools for investigating nonlinear partial differential equations (NLPDEs). These findings have potential applications in fields like fluid flow modeling, wave propagation in plasmas, and the study of nonlinear optical phenomena in physics and applied mathematics.

在本研究中,我们提出了分数耦合德林费尔德-索科洛夫-威尔逊(FCDSW)方程的孤波解的综合方法,该方程是一种通用数学模型,在流体动力学、等离子体物理学和非线性动力学中有着重要应用。通过利用最近开发的两种计算方法,即修正的萨达尔子方程(MSSE)方法和改进的(mathbb {F})扩展方法,我们以暗、暗-亮、亮-暗、奇异、周期、指数和有理的形式展示了新颖的孤子解。此外,我们还提取了 W 形、V 形、混合三角函数形和双曲形的孤子波解,这些都是以前未曾报道过的。此外,我们还研究了所提模型的调制不稳定性(MI)。为了进一步了解 FCDSW 方程的动力学,我们进行了详细的分岔分析,以研究这些方程表现出的分岔事件。我们还进行了敏感性分析,以评估模型对初始条件和参数变化的稳健性,从而为了解系统对扰动的敏感性提供有价值的见解。我们利用分析工具和数值模拟证明了所建议的技术在分析 FCDSW 方程中的有效性。我们的结果为 FCDSW 方程的行为和解法提供了新的见解,并增强了研究非线性偏微分方程 (NLPDE) 的数学工具。这些发现有望应用于流体流动建模、等离子体中的波传播以及物理学和应用数学中的非线性光学现象研究等领域。
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引用次数: 0
Quantum Visual Secret Sharing Based on Position Superposition 基于位置叠加的量子视觉秘密共享
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-28 DOI: 10.1007/s10773-024-05753-1
Meng-Yuan Zhao, Zi-Ming Wu, Bin Yan, Jeng-Shyang Pan, Hong-Mei Yang

Quantum visual secret sharing scheme combines the traditional visual secret sharing scheme with quantum properties to improve the security of secret information. However, all existing quantum visual secret sharing schemes encode a single pixel as a quantum superposition state. Each pixel requires n qubits for encoding. The number of qubits required grows proportionally to the number of pixels, which is unfavorable when the secret image is large. To reduce the number of qubits used, we propose a (n, n)-threshold quantum visual secret sharing scheme based on position superposition. In the secret sharing phase, the position and the encoded color corresponding to the position of the image are encoded as a quantum superposition state simultaneously. The whole secret image is encoded only once instead of encoding individual pixels. Only (varvec{2m+n}) qubits are required for a secret image of size (varvec{2^m times 2^m}). Then, the qubits encoding the position and the color of the secret image are distributed to n participants. In the recovery phase, n participants work together to recover the secret image by a quantum XOR operation on the qubits encoding the color. Simulations have been carried out to verify the practical feasibility of this scheme. Our scheme reduces the number of qubits used in the secret sharing process compared to previous quantum visual secret sharing schemes. In addition, there is no need to design the codebook in advance and the secret image can be fully recovered.

量子视觉秘密共享方案将传统的视觉秘密共享方案与量子特性相结合,以提高秘密信息的安全性。然而,所有现有的量子视觉秘密共享方案都将单个像素点编码为量子叠加态。每个像素需要 n 个量子比特进行编码。所需的量子比特数与像素数成正比增长,这在秘密图像较大时是不利的。为了减少使用的量子比特数,我们提出了一种基于位置叠加的(n,n)阈值量子视觉秘密共享方案。在秘密共享阶段,与图像位置相对应的位置和编码颜色被同时编码为量子叠加态。整个秘密图像只编码一次,而不是对单个像素进行编码。对于大小为 (varvec{2^m ×times 2^m}) 的秘密图像,只需要 (varvec{2m +n}) 量子比特。然后,编码秘密图像的位置和颜色的量子比特被分配给 n 个参与者。在恢复阶段,n 个参与者通过对编码颜色的量子比特进行量子 XOR 运算,共同恢复秘密图像。我们进行了仿真,以验证该方案的实际可行性。与之前的量子视觉秘密共享方案相比,我们的方案减少了秘密共享过程中使用的量子比特数量。此外,无需事先设计编码本,秘密图像也可以完全恢复。
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引用次数: 0
Three Dimensional Exploration of the Dynamics of Bell Diagonal States 贝尔对角线状态动力学的三维探索
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-27 DOI: 10.1007/s10773-024-05731-7
Varsha Sambhaje, Anju Chaurasia

Within the framework of quantum information theory, the performance of conventional 2-D techniques is often unsatisfactory for the study of Bell states that hold a unique status as maximally entangled states. Therefore, 3-D approaches are increasingly employed to achieve more accurate and detailed analysis, offering improved performance and insights in complex scenarios. Among the diverse background of mixed two-qubit states, certain configurations exhibit unique quantum correlations that harness advanced quantum information processing tasks such as Bell diagonal states. Although, these states may appear superficially simple and exhibit a rich spectrum of correlations. The present research employs a methodology that involves a convex combination of distinct Bell states to generate the entire class of Bell diagonal states. This work explores the time evolution of Bell diagonal states, when exposed to various quantum channels and investigates the dynamics of quantum correlations such as entanglement, discord, and state of separability. Finally, the behaviour of Bell diagonal states is analysed and results are compared between theory and practice. A threedimensional visual approach is used to illustrate a deeper understanding of various quantum features and dynamic behaviour of the Bell diagonal states.

在量子信息论的框架内,传统二维技术的性能往往无法满足对贝尔态的研究,因为贝尔态具有最大纠缠态的独特地位。因此,人们越来越多地采用三维方法来实现更精确、更详细的分析,从而在复杂情况下提高性能和洞察力。在混合双量子比特态的各种背景中,某些配置表现出独特的量子相关性,可以利用贝尔对角态等先进的量子信息处理任务。虽然这些态表面上看似简单,但却表现出丰富的相关性。目前的研究采用了一种方法,将不同的贝尔态进行凸组合,生成整个贝尔对角态类别。这项工作探索了贝尔对角线态暴露于各种量子通道时的时间演化,并研究了量子相关性的动态,如纠缠、不和谐和可分离状态。最后,对贝尔对角态的行为进行了分析,并对理论和实践结果进行了比较。该书采用三维可视化方法来说明对贝尔对角线态的各种量子特征和动态行为的深入理解。
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引用次数: 0
On the Degrees of Freedom Count on Singular Phase Space Submanifolds 论奇异相空间子曼形上的自由度计数
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-26 DOI: 10.1007/s10773-024-05741-5
Alexey Golovnev

I discuss singular loci in the phase spaces of theories which lack globally well-defined numbers of dynamical modes. This is a topic which appears quite often in the recent literature on modified gravity. In particular, there were discussions about (R^2) gravity around Minkowski space. It is a relatively simple case, and still there were some confusions. It clearly shows that one should be very accurate when trying to understand a potentially problematic theory through perturbations around a simply looking background. At the same time, many modern teleparallel approaches are laden with even more severe issues. Therefore, it is a topic which is certainly worth carefully thinking about.

我将讨论缺乏全局定义良好的动力学模式数的理论相空间中的奇异位置。这是最近关于修正引力的文献中经常出现的一个话题。特别是关于闵科夫斯基空间周围的(R^2)引力的讨论。这是一个相对简单的案例,但仍然存在一些困惑。这清楚地表明,当我们试图通过围绕简单背景的扰动来理解一个可能有问题的理论时,应该非常准确。与此同时,许多现代远距平行方法都存在着更为严重的问题。因此,这无疑是一个值得认真思考的课题。
{"title":"On the Degrees of Freedom Count on Singular Phase Space Submanifolds","authors":"Alexey Golovnev","doi":"10.1007/s10773-024-05741-5","DOIUrl":"https://doi.org/10.1007/s10773-024-05741-5","url":null,"abstract":"<p>I discuss singular loci in the phase spaces of theories which lack globally well-defined numbers of dynamical modes. This is a topic which appears quite often in the recent literature on modified gravity. In particular, there were discussions about <span>(R^2)</span> gravity around Minkowski space. It is a relatively simple case, and still there were some confusions. It clearly shows that one should be very accurate when trying to understand a potentially problematic theory through perturbations around a simply looking background. At the same time, many modern teleparallel approaches are laden with even more severe issues. Therefore, it is a topic which is certainly worth carefully thinking about.</p>","PeriodicalId":597,"journal":{"name":"International Journal of Theoretical Physics","volume":null,"pages":null},"PeriodicalIF":1.4,"publicationDate":"2024-08-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142209445","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Higgs Boson Decay into $$D^{*pm }$$ Meson Via Fragmentation 希格斯玻色子通过碎片衰变为 $$D^{*pm }$ 介子
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-26 DOI: 10.1007/s10773-024-05755-z
T. Osati, H. Pegah

The standard model Higgs boson has various decay modes, some of which have been measured in the CMS and ATLAS experiments, located at the Large Hadron Collider at CERN. This paper, calculates the decay of the standard model Higgs boson into (D^{*pm }) meson through the mechanism direct fragmentation. In this approach, the Higgs boson, first decays into (cbar{c}) and (bbar{b}) pairs, and then the heavy quarks fragment directly into (D^{*pm }) meson. The branching ratios of the SM Higgs boson into (D^{*pm }) meson have been calculated by considering NLO and NNLO corrections in the fragmentation functions of (D^{*pm }).

标准模型希格斯玻色子有多种衰变模式,位于欧洲核子研究中心大型强子对撞机上的CMS和ATLAS实验已经测量到了其中一些衰变模式。本文计算了标准模型希格斯玻色子通过直接碎片机制衰变成介子的过程。在这种方法中,希格斯玻色子首先衰变成(c)和(b)对,然后重夸克直接碎裂成(D^{*pm })介子。通过考虑 (D^{*pm }) 碎片函数中的 NLO 和 NNLO 修正,计算了 SM 希格斯玻色子进入 (D^{*pm }) 介子的分支率。
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引用次数: 0
Investigation of Space-Time Dynamics of Akbota Equation using Sardar Sub-Equation and Khater Methods: Unveiling Bifurcation and Chaotic Structure 使用 Sardar 子方程和 Khater 方法研究 Akbota 方程的时空动力学:揭示分岔和混沌结构
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-22 DOI: 10.1007/s10773-024-05733-5
Muhammad Moneeb Tariq, Muhammad Bilal Riaz, Muhammad Aziz-ur-Rehman

This paper focuses on obtaining exact solutions of nonlinear Akbota equation through the application of the modified Khater method and Sardar sub-equation method. Renowned as one of the latest and precise analytical schemes for nonlinear evolution equations, this method has proven its efficacy by generating diverse solutions for the model under consideration. The equation is crucial in the study of optical solitons, which are stable pulses of light that maintain their shape over long distances. The Akbota equation helps in understanding the behavior and stability of these solitons. The governing equation undergoes transformation into an ordinary differential equation through a well-suited wave transformation. This analytical simplification paves the way for the derivation of trigonometric, hyperbolic, and rational solutions through the proposed methods. To illuminate the physical behavior of the model, the study presents graphical plots of the selected solutions of Khater and Sardar sub-equation method. This visual representation, achieved by selecting appropriate values for arbitrary parameters, enhances the understanding of the system’s dynamics. All calculations in this study are meticulously conducted using the Mathematica and Maple software, ensuring accuracy and reliability in the analysis of the obtained solution. Furthermore we investigate the sensitivity analysis of the dynamical system.

本文的重点是通过应用改进的 Khater 方法和 Sardar 子方程方法,获得非线性 Akbota 方程的精确解。该方法被誉为非线性演化方程的最新精确分析方案之一,它为所考虑的模型生成了多种解,证明了其有效性。该方程对于研究光孤子至关重要,光孤子是一种稳定的光脉冲,能在长距离内保持其形状。阿克波塔方程有助于理解这些孤子的行为和稳定性。通过适当的波变换,支配方程被转化为常微分方程。这种分析上的简化为通过所提出的方法推导出三角、双曲和有理解铺平了道路。为了阐明模型的物理行为,本研究展示了 Khater 和 Sardar 子方程法所选解法的图形图。通过为任意参数选择适当的值,实现了这种直观表示,从而加深了对系统动力学的理解。本研究中的所有计算均使用 Mathematica 和 Maple 软件进行,以确保所得解分析的准确性和可靠性。此外,我们还研究了动态系统的敏感性分析。
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引用次数: 0
Leveraging Grover’s Algorithm for Quantum Searchable Encryption in Cloud Infrastructure and its application in AES Resource Estimation 利用格罗弗算法实现云基础设施中的量子可搜索加密及其在 AES 资源估算中的应用
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-21 DOI: 10.1007/s10773-024-05751-3
Mohit Joshi, Manoj Kumar Mishra, S. Karthikeyan

Designing efficient techniques to search over encrypted data space has always been an intriguing security challenge, although many solutions based on classical searching methods have been proposed. Grover’s algorithm, a quantum counterpart of searching algorithms, has proven to provide quadratic speedup over any classical search technique on an unsorted database. However, this algorithm is unable to search over encrypted data space. This study proposed an extension of Grover’s algorithm to enable search over encrypted dataspace, allowing clients with limited-capability quantum resources to delegate complex search operations to an untrusted server. The blindness of data in this protocol is achieved by encrypting qubits using Pauli’s rotation gates that maximally mix the outgoing states. The empirical estimation of the overhead of the computation due to the introduction of this technique has been analyzed. This estimate has been used for comparative analysis, showing the efficiency of the proposed protocol. A practical application of the proposed searchable encryption technique has been utilized to estimate the increase in resources needed to carry out a brute-force attack on AES encryption using secure Grover’s algorithm. Furthermore, an extensive experimental analysis of the effect of noise has been studied using four different noise models: amplitude damping, phase damping, depolarizing noise, and bit-flip noise. The investigation provided useful insight into the behavior of the proposed algorithm under noisy conditions and also estimated the tolerance thresholds of the proposed algorithm under different noise models.

尽管已经提出了许多基于经典搜索方法的解决方案,但设计高效的加密数据空间搜索技术一直是一个引人入胜的安全挑战。格罗弗算法是搜索算法的量子对应算法,已被证明在无排序数据库上比任何经典搜索技术都有四倍的速度提升。然而,这种算法无法在加密数据空间上进行搜索。本研究提出了对格罗弗算法的扩展,以实现对加密数据空间的搜索,从而允许能力有限的量子资源客户端将复杂的搜索操作委托给不受信任的服务器。该协议中的数据盲区是通过使用保利旋转门加密量子比特来实现的,这种旋转门能最大限度地混合传出状态。我们分析了因引入这种技术而产生的计算开销的经验估计值。这一估算结果被用于比较分析,显示了所提协议的效率。利用所提出的可搜索加密技术的实际应用,估算了使用安全格罗弗算法对 AES 加密进行暴力破解所需的资源增加量。此外,还利用四种不同的噪声模型对噪声的影响进行了广泛的实验分析:振幅阻尼、相位阻尼、去极化噪声和比特翻转噪声。这项研究为了解拟议算法在噪声条件下的行为提供了有用的见解,还估算了拟议算法在不同噪声模型下的容限阈值。
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引用次数: 0
Dynamics of a Perturbed Higher Dimensional Black Hole with Exponential Entropy in the Framework of Einstein-Yang-Mills Gravity 爱因斯坦-杨-米尔斯引力框架下具有指数熵的受扰动高维黑洞的动力学
IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-21 DOI: 10.1007/s10773-024-05750-4
Khaja Zuber Amin, Prince A. Ganai

We investigate the thermodynamic properties of a five-dimensional Reissner-Nordström black hole within the framework of Einstein-Yang-Mills gravity, employing the higher-dimensional Wu-Yang Ansatz. By incorporating quantum fluctuations, we examine the behavior of thermodynamic potentials, including internal energy, free energy, Gibbs free energy, and enthalpy. Our analysis reveals that quantum effects are predominantly influential near the event horizon, with negligible impact on larger black holes. Notably, Gibbs free energy emerges as a promising candidate for modeling the black hole as a heat engine. Furthermore, specific heat analysis indicates a second-order phase transition for the system under consideration.

我们在爱因斯坦-杨-米尔斯引力的框架内,采用高维吴-杨解析,研究了五维赖斯纳-诺德斯特伦黑洞的热力学性质。通过纳入量子波动,我们研究了热力学势的行为,包括内能、自由能、吉布斯自由能和焓。我们的分析表明,量子效应主要影响事件穹界附近,对较大黑洞的影响可以忽略不计。值得注意的是,吉布斯自由能是将黑洞建模为热机的一个有前途的候选方案。此外,比热分析表明所考虑的系统存在二阶相变。
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引用次数: 0
期刊
International Journal of Theoretical Physics
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