Properties of expanding universes
Some implications and consequences of the expansion of the universe are examined. In Chapter 1 it is shown that this expansion creates grave difficulties for the Hoyle-Narlikar theory of gravitation. Chapter 2 deals with perturbations of an expanding homogeneous and isotropic universe. The conclusio...
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ndltd-bl.uk-oai-ethos.bl.uk-6011532017-12-24T15:13:56ZProperties of expanding universesHawking, Stephen1966Some implications and consequences of the expansion of the universe are examined. In Chapter 1 it is shown that this expansion creates grave difficulties for the Hoyle-Narlikar theory of gravitation. Chapter 2 deals with perturbations of an expanding homogeneous and isotropic universe. The conclusion is reached that galaxies cannot be formed as a result of the growth of perturbations that were initially small. The propagation and absorption of gravitational radiation is also investigated in this approximation. In Chapter 3 gravitational radiation in an expanding universe is examined by a method of asymptotic expansions. The 'peeling off' behaviour and the asymptotic group are derived. Chapter 4 deals with the occurrence of singularities in cosmological models. It is shown that a singularity is inevitable provided that certain very general conditions are satisfied.500CosmologyUniversity of Cambridge10.17863/CAM.11283http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.601153https://www.repository.cam.ac.uk/handle/1810/251038Electronic Thesis or Dissertation |
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500 Cosmology |
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500 Cosmology Hawking, Stephen Properties of expanding universes |
description |
Some implications and consequences of the expansion of the universe are examined. In Chapter 1 it is shown that this expansion creates grave difficulties for the Hoyle-Narlikar theory of gravitation. Chapter 2 deals with perturbations of an expanding homogeneous and isotropic universe. The conclusion is reached that galaxies cannot be formed as a result of the growth of perturbations that were initially small. The propagation and absorption of gravitational radiation is also investigated in this approximation. In Chapter 3 gravitational radiation in an expanding universe is examined by a method of asymptotic expansions. The 'peeling off' behaviour and the asymptotic group are derived. Chapter 4 deals with the occurrence of singularities in cosmological models. It is shown that a singularity is inevitable provided that certain very general conditions are satisfied. |
author |
Hawking, Stephen |
author_facet |
Hawking, Stephen |
author_sort |
Hawking, Stephen |
title |
Properties of expanding universes |
title_short |
Properties of expanding universes |
title_full |
Properties of expanding universes |
title_fullStr |
Properties of expanding universes |
title_full_unstemmed |
Properties of expanding universes |
title_sort |
properties of expanding universes |
publisher |
University of Cambridge |
publishDate |
1966 |
url |
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.601153 |
work_keys_str_mv |
AT hawkingstephen propertiesofexpandinguniverses |
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1718566784407175168 |