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Usman Thermal Stability and Hawking Evaporation of Specific Black Holes

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dc.contributor.author Zafar, Usman
dc.date.accessioned 2022-08-22T08:59:24Z
dc.date.available 2022-08-22T08:59:24Z
dc.date.issued 2022-08-22
dc.identifier.uri http://repository.cuilahore.edu.pk/xmlui/handle/123456789/3438
dc.description.abstract In this thesis, we explore thermal fluctuations for different black holes such as braneworld black hole and Renormalization group improved Schwarz schild black hole. Thermodynamic quantities such as temperature, pressure, entropy, specific heat capacity at constant pressure and volume, ratio be tween these heat capacities, Gibbs free energy and Helmholtz free energy are discussed for these black holes. To investigate the stability condition of these black holes, exponential corrected entropy has been used. Local and global stability of these black holes in canonical ensemble and grand canonical ensemble are being explored. We investigate the Hawking evapo ration of Reisner Nordst¨orm anti-de-Sitter black hole with global monopole and anti-de-Sitter charged black hole with global monopole. We derive and plot the metric function, effective potential, mass and Hawking tempera ture of these black holes and also discuss the effects of these quantities on the Hawking evaporation of these black holes. Lifetime of these black holes and how the evaporation process is make faster or slower are discussed. en_US
dc.language.iso en en_US
dc.publisher Mathematics COMSATS University Islamabad Lahore Campus en_US
dc.relation.ispartofseries ;SP20-RMT-014
dc.subject Evaporation process, energy and Helmholtz en_US
dc.title Usman Thermal Stability and Hawking Evaporation of Specific Black Holes en_US
dc.type Thesis en_US


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  • Thesis - MS / PhD
    This collection containts the Ms/PhD theses of the studetns of Mathematics Department

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