Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes

EMU I-REP

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dc.contributor.advisor Sakallı, İzzet (Supervisor)
dc.contributor.author Sucu, Erdem
dc.date.accessioned 2025-06-04T11:51:11Z
dc.date.available 2025-06-04T11:51:11Z
dc.date.issued 2024-01
dc.date.submitted 2024-01
dc.identifier.citation Sucu, Erdem. (2024). Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes. 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/11129/6335
dc.description Master of Science in Physics. Institute of Graduate Studies and Research. Thesis (M.S.) - Eastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physics, 2024. Supervisor: Prof. Dr. İzzet Sakallı en_US
dc.description.abstract The impact of the Generalized Uncertainty Principle (GUP) on Hawking particle emission in a rotating linear dilaton black hole (RLDBH) spacetime is examined in this thesis. The concerned study presents a thermal emission model for black holes (BHs) that incorporates the influence of gravitational lens particles through GUP during the quantum tunneling process. The findings suggest that with GUP support, the temperature of Hawking radiation decreases as GUP parameters increase and rises with an increasing BH mass. The thesis also delves into the repercussions of these discoveries on the information loss paradox and adjusted entropy, while also exploring the potential utilization of astrophysical data to confirm GUP effects. In conclusion, our work underscores the significant role of GUP in the thermal emission of non-asymptotically flat (NAF), stationary BHs and its capacity to shed light on the intricate relationship between astrophysics and quantum gravity. en_US
dc.description.abstract ÖZ: Bu tezde, genelle¸stirilmi¸s belirsizlik ilkesi’nin (GUP), dönen dogrusal dilaton kara ˘ delik uzayzamanında Hawking parçacık emisyonu üzerindeki etkisi incelenmektedir. Bu çalı¸sma, kütleçekim mercek parçacıklarının GUP aracılıgıyla kuantum tünelleme ˘ sürecindeki etkisini içeren kara delikler için bir termal emisyon modeli sunulmaktadır. Elde edilen bulgular, GUP destegi ile Hawking radyasyonunun ˘ sıcaklıgının GUP parametreleri arttıkça azaldı ˘ gını ve artan siyah delik kütleleri ile ˘ arttıgını önermektedir. Tez ayrıca bu ke¸siflerin bilgi kaybı paradoksu ve ayarlanmı¸s ˘ entropi üzerindeki etkilerini incelemekte ve aynı zamanda GUP etkilerini dogrulamak ˘ için astrofizik verilerinin potansiyel kullanımını ara¸stırmaktadır. Sonuç olarak, çalı¸smamız, GUP’un asimptotik olarak düz olmayan, duragan kara deliklerin termal ˘ emisyonunda oynadıgı önemli rolü ve astrofizik ile kuantum kütleçekimi arasındaki ˘ karma¸sık ili¸skiyi aydınlatma kapasitesini vurgulamaktadır. 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 Department en_US
dc.subject Black Holes--Physics en_US
dc.subject Radiation en_US
dc.subject Astronomy en_US
dc.subject Astrophysics en_US
dc.subject Universe en_US
dc.subject Space and Time en_US
dc.subject Hawking Radiation, GUP, Linear Dilaton, Quantum Tunneling, Black holes en_US
dc.title Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes 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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