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In this project, we analyze Kerr-de Sitter metric in higher dimensions, up to eleven dimensions. General relativity will be introduced, including tensors linked to the curvature of spacetime, along with de Sitter metric. de Sitter metric will be pre-determined as background metric to get simple expl...

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Main Author: (NIM : 10213091), RAMADHIANSYAH
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/23823
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:23823
spelling id-itb.:238232017-11-09T10:08:44Z#TITLE_ALTERNATIVE# (NIM : 10213091), RAMADHIANSYAH Indonesia Final Project INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/23823 In this project, we analyze Kerr-de Sitter metric in higher dimensions, up to eleven dimensions. General relativity will be introduced, including tensors linked to the curvature of spacetime, along with de Sitter metric. de Sitter metric will be pre-determined as background metric to get simple explicit exact solution of the Einstein vacuum equations, called Kerr metric, with needed variables. Next, Kerr-Schild form of higher dimensional Kerr-de Sitter metric will be derived from general Kerr-de Sitter metrics, up to eleven dimensions. Afterwards, we will obtain identity tensors which are related to space-time curvature, they are metric tensors, Christoffel symbols, Riemann tensors, and Ricci tensors. From Ricci tensor of de Sitter background metric, we will get Ricci tensor of the exact Kerr-de Sitter metric. Furthermore, it will be used to obtain Ricci scalar and Einstein tensor of Kerr-de Sitter metric. 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 In this project, we analyze Kerr-de Sitter metric in higher dimensions, up to eleven dimensions. General relativity will be introduced, including tensors linked to the curvature of spacetime, along with de Sitter metric. de Sitter metric will be pre-determined as background metric to get simple explicit exact solution of the Einstein vacuum equations, called Kerr metric, with needed variables. Next, Kerr-Schild form of higher dimensional Kerr-de Sitter metric will be derived from general Kerr-de Sitter metrics, up to eleven dimensions. Afterwards, we will obtain identity tensors which are related to space-time curvature, they are metric tensors, Christoffel symbols, Riemann tensors, and Ricci tensors. From Ricci tensor of de Sitter background metric, we will get Ricci tensor of the exact Kerr-de Sitter metric. Furthermore, it will be used to obtain Ricci scalar and Einstein tensor of Kerr-de Sitter metric.
format Final Project
author (NIM : 10213091), RAMADHIANSYAH
spellingShingle (NIM : 10213091), RAMADHIANSYAH
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author_facet (NIM : 10213091), RAMADHIANSYAH
author_sort (NIM : 10213091), RAMADHIANSYAH
title #TITLE_ALTERNATIVE#
title_short #TITLE_ALTERNATIVE#
title_full #TITLE_ALTERNATIVE#
title_fullStr #TITLE_ALTERNATIVE#
title_full_unstemmed #TITLE_ALTERNATIVE#
title_sort #title_alternative#
url https://digilib.itb.ac.id/gdl/view/23823
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