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The Ricci flow, which connects metric evolution and curvature of space, was introduced by Richard Hamilton in 1982 in order to gain insight into the geometrization conjecture of William Thurston, concerning the topological classification of three dimensional smooth manifolds. In this thesis, we stud...

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Main Author: TAUFIK AKBAR (NIM. 20208017), FIKI
Format: Theses
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/12122
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:12122
spelling id-itb.:121222017-09-27T14:40:57Z#TITLE_ALTERNATIVE# TAUFIK AKBAR (NIM. 20208017), FIKI Indonesia Theses INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/12122 The Ricci flow, which connects metric evolution and curvature of space, was introduced by Richard Hamilton in 1982 in order to gain insight into the geometrization conjecture of William Thurston, concerning the topological classification of three dimensional smooth manifolds. In this thesis, we study some aspects of perturbative solutions of Ricci flow equation in four dimensional spacetime that admits a spherical symmetric metric. Two cases are considered, namely Ricci flat and Einstein metric cases. Then, we derive the surface gravity for both cases. We find that in both cases, surface gravity does not depend on a parameter T (tau). 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 The Ricci flow, which connects metric evolution and curvature of space, was introduced by Richard Hamilton in 1982 in order to gain insight into the geometrization conjecture of William Thurston, concerning the topological classification of three dimensional smooth manifolds. In this thesis, we study some aspects of perturbative solutions of Ricci flow equation in four dimensional spacetime that admits a spherical symmetric metric. Two cases are considered, namely Ricci flat and Einstein metric cases. Then, we derive the surface gravity for both cases. We find that in both cases, surface gravity does not depend on a parameter T (tau).
format Theses
author TAUFIK AKBAR (NIM. 20208017), FIKI
spellingShingle TAUFIK AKBAR (NIM. 20208017), FIKI
#TITLE_ALTERNATIVE#
author_facet TAUFIK AKBAR (NIM. 20208017), FIKI
author_sort TAUFIK AKBAR (NIM. 20208017), FIKI
title #TITLE_ALTERNATIVE#
title_short #TITLE_ALTERNATIVE#
title_full #TITLE_ALTERNATIVE#
title_fullStr #TITLE_ALTERNATIVE#
title_full_unstemmed #TITLE_ALTERNATIVE#
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url https://digilib.itb.ac.id/gdl/view/12122
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