هندسه‌ی ترمودینامیک سیاهچاله‌ی ‏AdS‏ باردار با آنتروپی تصحیح یافته ‏

سروش فر, صاحب; پورحسن, بهنام

doi:10.22055/jrmbs.2021.17029

هندسه‌ی ترمودینامیک سیاهچاله‌ی ‏AdS‏ باردار با آنتروپی تصحیح یافته ‏

نوع مقاله : مقاله پژوهشی کامل

نویسندگان

¹ گروه فیزیک، دانشکده صنعت و معدن، دانشگاه یاسوج، چرام 7576159836، ایران

² گروه هسته ای و فیزیک ذرات بنیادی، دانشکده فیزیک، دانشگاه دامغان، دامغان، ایران.

10.22055/jrmbs.2021.17029

چکیده

در این مقاله، سیاهچاله‌ی پاد دو سیته (‏‎(AdS‏ باردار در نظر گرفته شده و تصحیحات نمایی آنتروپی آن مطالعه شده‌است. پس ‏از آن، کمیت‌های ترمودینامیکی این سیاهچاله شامل جرم، دما، ظرفیت گرمایی و همچنین فشار و انرژی آزاد گیبس، مورد ‏بررسی قرار گرفته‌اند. سپس، هندسه‌ی ترمودینامیک این سیاهچاله به کمک روش های هندسی وینهلد، راپینر، کوودو، اچ پی ‏ای ام و ان تی جی، بررسی شده است. علاوه براین، تناظر بین تکینگی‌های خمش متریک‌های هندسی و نقاط گذار فاز ‏سیاهچاله، مورد بررسی قرار گرفته‌است. مشاهده شده است که فرمالیسم‌های کوودو(‏II‏)، اچ پی ای ام و ان تی جی، اطلاعات ‏کاملتری را در خصوص نقاط گذار فاز این سیاهچاله نسبت به فرمالیسم‌های وینهولد، راپینر و کوودو(‏I‏)، ارائه می دهند.‏

کلیدواژه‌ها

موضوعات

گرانش و کیهانشناسی

عنوان مقاله [English]

Thermodynamic geometry of a charged AdS black hole ‎with corrected entropy

نویسندگان [English]

Saheb Soroushfar ¹
Behnam Pourhassan ²

¹ Department of Physics, Faculty of Technology and Mining, Yasouj University, Choram 75761-59836, Iran

² School of Physics, Damghan University, Damghan, 3671641167, Iran

چکیده [English]

In this paper, a charged AdS black hole is considered and exponential corrections on entropy ‎are studied for it. Next, thermodynamic quantities of this black hole, including mass, ‎temperature, heat capacity, as well as pressure and Gibbs free energy, are investigated. Then, ‎the thermodynamic geometry of this black hole is investigated using the geometric methods of ‎Weinhold, Ruppeiner, Quevedo, HPEM and NTG. In addition, the correspondence between ‎singularities of the scalar curvature of these metrics and the black hole phase transition points ‎is investigated. It has been observed that Quevedo (II), HPEM and NTG formalisms provide ‎more information about the phase transition of this black hole compared with Weinhold, ‎Ruppeiner and Quevedo (I) formalisms.‎

کلیدواژه‌ها [English]

Black hole
Thermodynamics
Thermodynamic geometry
Phase transition

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