English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

This thesis mainly focuses on the Hawking radiation (HR) evacuating from thesurface of the objects that have earned a reputation as the most extraordinaryobjects existing so far; the black holes (BHs). Throughout this study, quantumtunneling (QT) process serves as the model for the HR of scalar, vector andDirac particles. The scalar and Dirac particles are anticipated to be tunnelingthrough the horizon of rotating scalar hairy black holes (RHSBHs); whilst thevector particles are associated with a rotating warped anti de-Sitter blackhole (WAdS3BH) embedded in a (2+1) dimensional fabric. It is no coincidencethat for all three cases; the standard HT expression is derived. Additionally,the engagement of conformal field theory (CFT) with anti de-Sitter (AdS) spacepresents itself to the reader and the methodologies of Klein-Gordon equation(KGE), Dirac equation and Proca equations (PEs) are introduced. For all threecases, Hamilton-Jacobi (HJ) approach is used, together withWentzel-Kramers-Brillouin (WKB) Approximation. Finally, the BH structures arecompared with thermodynamics to derive HT with the aid of Boltzmann factor.

Hawking Radiation of Warped Anti de Sitter and Rotating Hairy Black Holes with Scalar Hair