Rendering dark energy void

Rendering dark energy void

Includes abstract. === Includes bibliographical references (leaves 114-120). === The current model of cosmology, the Friedman-Lemaitre-Robertson-Valker model, assumes that the universe is approximately homogeneous and isotropic on very large scales. Further assuming flatness and dark energy in the f...

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Bibliographic Details
Main Author: February, Sean Phillip
Other Authors: Clarkson, Chris
Format: Dissertation
Language:English
Published: University of Cape Town 2015
Subjects:
Cosmology
Online Access:http://hdl.handle.net/11427/11912
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spelling ndltd-netd.ac.za-oai-union.ndltd.org-uct-oai-localhost-11427-119122020-10-06T05:11:41Z Rendering dark energy void February, Sean Phillip Clarkson, Chris Cosmology Includes abstract. Includes bibliographical references (leaves 114-120). The current model of cosmology, the Friedman-Lemaitre-Robertson-Valker model, assumes that the universe is approximately homogeneous and isotropic on very large scales. Further assuming flatness and dark energy in the form of Einstein's cosmological constant A then implies that the latter contributes roughly 73% of the total energy of the universe, cold dark matter (CD'I) 23SiC, and baryons, the matter we are made, only 4%. 2015-01-10T06:56:47Z 2015-01-10T06:56:47Z 2009 Master Thesis Masters MSc http://hdl.handle.net/11427/11912 eng application/pdf University of Cape Town Faculty of Science Department of Astronomy
collection NDLTD
language English
format Dissertation
sources NDLTD
topic Cosmology
spellingShingle Cosmology
February, Sean Phillip
Rendering dark energy void
description Includes abstract. === Includes bibliographical references (leaves 114-120). === The current model of cosmology, the Friedman-Lemaitre-Robertson-Valker model, assumes that the universe is approximately homogeneous and isotropic on very large scales. Further assuming flatness and dark energy in the form of Einstein's cosmological constant A then implies that the latter contributes roughly 73% of the total energy of the universe, cold dark matter (CD'I) 23SiC, and baryons, the matter we are made, only 4%.
author2 Clarkson, Chris
author_facet Clarkson, Chris
February, Sean Phillip
author February, Sean Phillip
author_sort February, Sean Phillip
title Rendering dark energy void
title_short Rendering dark energy void
title_full Rendering dark energy void
title_fullStr Rendering dark energy void
title_full_unstemmed Rendering dark energy void
title_sort rendering dark energy void
publisher University of Cape Town
publishDate 2015
url http://hdl.handle.net/11427/11912
work_keys_str_mv AT februaryseanphillip renderingdarkenergyvoid
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