Hawking Radiation of Rindler Modified Schwarzschild Black Hole

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dc.contributor.author Yakub, Sherwan Kher Al-Den
dc.date.accessioned 2015-03-17T08:24:11Z
dc.date.available 2015-03-17T08:24:11Z
dc.date.issued 2014-07
dc.identifier.citation Yakub, Sherwan Kher Al-Den. (2014). Hawking Radiation of Rindler Modified Schwarzschild Black Hole. 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/11129/1650
dc.description Master of Science in Physics. Thesis (M.S.)--Eastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physics, 2014. Supervisor: Assoc. Prof. Dr. İzzet Sakallı. en_US
dc.description.abstract ABSTRACT: One of the significant techniques to calculate the black hole (BH) temperature and understand BH thermodynamics is to employ the semi-classical BH tunneling method. In this thesis, by using the Parikh-Wilczek (PW), Hamilton-Jacobi (HJ) and Damour-Ruffini-Sannan (DRS) tunneling methods, we aim to explore the Hawking radiation (HR) of the Grumiller BH (GBH). This BH is also known as Rindler modified Schwarzschild BH. Generally, in the tunneling method the imaginary part of the action (classically forbidden process) is directly proportional to the Boltzmann factor or is inversely proportional to the temperature of the BH whose performing the Hawking radiation (HR). In the original work of PW, who considered the self-gravitational effect with the energy conservation, it was shown that the small deviations from pure thermal radiation in the HR may cause to a leakage of the information from the BH. This phenomenon is summarized and extended to the GBH in this dissertation. Keywords: Quantum tunneling method, Hawking radiation, Relativistic Hamilton-Jacobi equation, Parikh-Wilczek method, Damour-Ruffini-Sannan method, Grumiller black hole, Rindler acceleration. ………………………………………………………………………………………………………………………… ÖZ: Kara delik (BH) sıcaklığını hesaplamak ve BH termodinamiğini anlamak için en önemli tekniklerden birisi yarı-klasik BH tünelleme yöntemini kullanmaktır. Bu tezde, Parikh-Wilczek (PW), Hamilton-Jacobi (HJ) ve Damour-Ruffini-Sannan (DRS) tünelleme yöntemleri kullanarak, biz Grumiller BH (GBH)'un ve Hawking radyasyonunu (HR) araştırmayı hedefliyoruz. Bu BH, Rindler modifiyeli Schwarzschild BH'u olarak da bilinmektedir. Genel olarak, tünelleme yönteminde eylemin (klasik olarak yasaklanmış işlem) sanal kısmı Boltzmann faktörü ile doğrudan orantılıdır ya da Hawking radyasyon (HR) gerçekleştiren BH'un sıcaklığına ters orantılıdır. Enerji korunumu ile kendini yerçekimi etkisinin dikkate alındığı PW'in orjinal çalışmasında, HR'nın saf termal radyasyonundaki küçük sapmaların BH'dan bir bilgi sızıntısına neden olduğu gösterilmiştir. Bu olgu, bu tezde özetlenmiş ve GBH için genişletilmiştir. Anahtar kelimeler: Kuantum tünelleme metodu, Hawking radyasyonu, Relativisitik Hamilton-Jacobi denklemi, Parikh-Wilczek metodu, Damour-Ruffini-Sannan metodu, Grumiller kara deliği, Rindler ivmesi. en_US
dc.language.iso en en_US
dc.publisher Eastern Mediterranean University (EMU) - Doğu Akdeniz Üniversitesi (DAÜ) en_US
dc.subject Physics en_US
dc.subject Quantum theory en_US
dc.subject Quantum gravity en_US
dc.subject Space Physics en_US
dc.subject Quantum Tuneling Method, Hawking Radiation, Relativistic Hamilton-Jacobi Equation, Parikh-Wilczek Method, Damour-Ruffini-Sannan Method, Grumiller Black Hole, Rindler Acceleration en_US
dc.title Hawking Radiation of Rindler Modified Schwarzschild Black Hole en_US
dc.type Thesis en_US


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