Quantization of Euclidean Black Holes via the Adiabatic Invariance Method

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dc.contributor.advisor Sakallı, İzzet
dc.contributor.author Uğural, Esen
dc.date.accessioned 2020-11-26T12:54:17Z
dc.date.available 2020-11-26T12:54:17Z
dc.date.issued 2016
dc.date.submitted 2016
dc.identifier.citation Uğural, Esen. (2016). Quantization of Euclidean Black Holes via the Adiabatic Invariance Method. Thesis (M.S.), Eastern Mediterranean University, Institute of Graduate Studies and Research, Dept. of Physics, Famagusta: North Cyprus. en_US
dc.identifier.uri http://hdl.handle.net/11129/4769
dc.description Master of Science in Physics. Thesis (M.S.)--Eastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physics, 2016. Supervisor: Assoc. Prof. Dr. İzzet Sakallı. en_US
dc.description.abstract In this thesis, we calculate the entropy of four different types of black holes and show that entropy and area of the considered black holes are equally likely quantized. The quantization of entropy/area of the black holes are employed by using the adiabatic invariance formulation of the famous Bohr-Sommerfeld theory. Moreover, we consider the exactness conditions of the first order differential equations to derive the integral solution of the adiabatic invariance. The black holes that are going to be discussed are the Schwarzschild black hole, the Kerr black hole, the Reissner-Nordström black hole and the Kerr-Newman black hole. In particular, the detailed derivations of the adiabatic invariance`s integral solutions for the latter three black holes, are given. At the end of each chapter, the quantization of the entropy/area spectrum for the considered black hole is proven via the Bekenstein’s area conjecture. Keywords: Black hole, Black hole area, Black hole entropy, Adiabatic invariance, Exact differential equations, Quantization of black hole entropy and area. en_US
dc.description.abstract ÖZ: Bu tezde, dört farklı tür karadelik için entropi hesaplıyoruz ve ayrıca entropi ve alanın her ikisinin de benzer ve eşit şekilde kuantize olduğunu gösteriyoruz. Alan ve entropinin kuantize oldukları, Bohr-Sommerfeld’in ünlü adyabatik sabitlik formülasyonu kullanılarak gösteriliyor. Ayrıca, adyabatik sabit için integral hesaplamalarını yaparken kesin diferansiyel eşitlik çözümlerini de dikkate alıyoruz. İlgilendiğimiz karadelikler sırasıyla Schwarzschild karadeliği, Kerr karadeliği, Reissner-Nordström karadeliği ve Kerr-Newman karadeliğidir. Ayrıca, son üçünün adyabatik sabitlerinin ayrıntılı integral hesaplamaları veriliyor. Her bölümün sonunda, Bekenstein’ın alan varsayımı aracılığı ile, ele alınan kara delik için alan ve entropi tayfının kuantize oldukları doğrulanmıştır. Hesaplanmış olan entropi ile alan kıyaslanarak orantılı ve kuantize oldukları gösterilmektedir. Anahtar kelimeler: Karadelik, Karadelik alanı, Karadelik entropisi, Adiyabatik sabitlik, Kesin diferansiyel eşitlik, Kuantize karadelik entropisi ve alanı. en_US
dc.language.iso eng en_US
dc.publisher Eastern Mediterranean University (EMU) - Doğu Akdeniz Üniversitesi (DAÜ) en_US
dc.rights info:eu-repo/semantics/openAccess en_US
dc.subject Physics en_US
dc.subject Black Holes en_US
dc.subject Black hole en_US
dc.subject Black hole area en_US
dc.subject Black hole entropy en_US
dc.subject Adiabatic invarianc en_US
dc.subject Exact differential equations en_US
dc.subject Quantization of black hole entropy and area en_US
dc.title Quantization of Euclidean Black Holes via the Adiabatic Invariance Method en_US
dc.type masterThesis en_US
dc.contributor.department Eastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physics en_US


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