Quantization of Euclidean Black Holes via the Adiabatic Invariance Method

dc.contributor.advisorSakallı, İzzet
dc.contributor.authorUğural, Esen
dc.date.accessioned2020-11-26T12:54:17Z
dc.date.available2020-11-26T12:54:17Z
dc.date.issued2016
dc.date.submitted2016
dc.departmentEastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physicsen_US
dc.descriptionMaster 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.abstractIn 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.abstractÖZ: 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.identifier.citationUğural, 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.urihttps://hdl.handle.net/11129/4769
dc.language.isoen
dc.publisherEastern Mediterranean University (EMU) - Doğu Akdeniz Üniversitesi (DAÜ)en_US
dc.relation.publicationcategoryTez
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectPhysicsen_US
dc.subjectBlack Holesen_US
dc.subjectBlack holeen_US
dc.subjectBlack hole areaen_US
dc.subjectBlack hole entropyen_US
dc.subjectAdiabatic invariancen_US
dc.subjectExact differential equationsen_US
dc.subjectQuantization of black hole entropy and areaen_US
dc.titleQuantization of Euclidean Black Holes via the Adiabatic Invariance Methoden_US
dc.typeMaster Thesis

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