CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR

Stationary black hole model first introduced by Kerr satisfies vacuum Einstein field equation with zero cosmological constant. As we know, our universe has non-zero cosmological constant. In this thesis, we consider a stationary black hole which satisfies non-zero cosmological constant Einstein fiel...

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Main Author: WILIARDY (NIM: 20215048), ABEDNEGO
Format: Theses
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/20678
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:20678
spelling id-itb.:206782017-09-27T14:41:06ZCHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR WILIARDY (NIM: 20215048), ABEDNEGO Indonesia Theses INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/20678 Stationary black hole model first introduced by Kerr satisfies vacuum Einstein field equation with zero cosmological constant. As we know, our universe has non-zero cosmological constant. In this thesis, we consider a stationary black hole which satisfies non-zero cosmological constant Einstein field equation. Furthermore, the metric has an arbitrary constant Ricci scalar which imply a non-zero Einstein field equation and could be interpreted as a stationary black hole which is placed in a non-vacuum de Sitter space. Characterization of geometry is to analyze manifold singularity including physical and coordinate singularity. Moreover, we show the formed horizon and the critical limit of the black hole. Analysis of black hole <br /> <br /> <br /> thermodynamics is also performed including the calculation of surface gravity and surface area of the black hole. text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
description Stationary black hole model first introduced by Kerr satisfies vacuum Einstein field equation with zero cosmological constant. As we know, our universe has non-zero cosmological constant. In this thesis, we consider a stationary black hole which satisfies non-zero cosmological constant Einstein field equation. Furthermore, the metric has an arbitrary constant Ricci scalar which imply a non-zero Einstein field equation and could be interpreted as a stationary black hole which is placed in a non-vacuum de Sitter space. Characterization of geometry is to analyze manifold singularity including physical and coordinate singularity. Moreover, we show the formed horizon and the critical limit of the black hole. Analysis of black hole <br /> <br /> <br /> thermodynamics is also performed including the calculation of surface gravity and surface area of the black hole.
format Theses
author WILIARDY (NIM: 20215048), ABEDNEGO
spellingShingle WILIARDY (NIM: 20215048), ABEDNEGO
CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
author_facet WILIARDY (NIM: 20215048), ABEDNEGO
author_sort WILIARDY (NIM: 20215048), ABEDNEGO
title CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
title_short CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
title_full CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
title_fullStr CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
title_full_unstemmed CHARACTERIZATION OF STATIONARY BLACK HOLE GEOMETRY WITH CONSTANT RICCI SCALAR
title_sort characterization of stationary black hole geometry with constant ricci scalar
url https://digilib.itb.ac.id/gdl/view/20678
_version_ 1821120230405963776