Joule-Thomson expansion for charged-AdS black hole with nonlinear electrodynamics and thermal fluctuations by using Barrow entropy

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Journal of High Energy Astrophysics Pub Date : 2024-09-10 DOI:10.1016/j.jheap.2024.09.003
Faisal Javed , G. Mustafa , G. Fatima , S.K. Maurya , Mansoor H. Alshehri , Iqra Mubeen
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Abstract

This paper investigates the complex interplay between charged anti-de Sitter black hole thermodynamic behavior and nonlinear electrodynamics. Strong insights are obtained by examining the impact of nonlinear electrodynamics on the Joule-Thomson expansion of charged black holes and assessing the thermal fluctuations with higher-order corrections in the context of Barrow entropy. The research shows the complex interactions influencing thermal properties from Joule-Thomson coefficients are affected by temperature, pressure, and changes in gas composition due to the effects of charges and nonlinear electrodynamics factors on inversion temperature and pressure. Furthermore, analyzing black hole isenthalpic curves provides important insights into the thermodynamic behavior of the system by highlighting discrete heating and cooling zones in the inversion curve. Significant effects of nonlinear dynamics on the thermodynamic parameters of the system are highlighted by the notable variations in the Helmholtz free energy, internal energy, enthalpy, and Gibbs free energy of charged anti-de Sitter black holes. By demonstrating the complex and captivating nature of these interactions, the paper concludes by emphasizing the significant influence of nonlinear dynamics on the thermodynamic parameters of charged black holes within the framework of Barrow entropy.

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利用巴罗熵对具有非线性电动力学和热波动的带电 AdS 黑洞进行焦耳-汤姆森扩展
本文研究了带电反德西特黑洞热力学行为与非线性电动力学之间复杂的相互作用。通过研究非线性电动力学对带电黑洞焦耳-汤姆森膨胀的影响,以及评估巴罗熵背景下具有高阶修正的热波动,本文获得了深刻的见解。研究表明,由于电荷和非线性电动力学因素对反转温度和压力的影响,焦耳-汤姆逊系数对热特性的复杂相互作用受到温度、压力和气体成分变化的影响。此外,通过分析黑洞等温线,反转曲线上的离散加热区和冷却区会更加突出,从而为了解系统的热力学行为提供重要信息。带电反德西特黑洞的赫尔姆霍兹自由能、内能、焓和吉布斯自由能的显著变化,凸显了非线性动力学对系统热力学参数的重要影响。通过展示这些相互作用复杂而迷人的性质,论文最后强调了在巴罗熵框架内非线性动力学对带电黑洞热力学参数的重要影响。
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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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