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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Main Author: Hawking, Stephen
Published: University of Cambridge 1966
Subjects:
500
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.601153
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spelling 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
collection NDLTD
sources NDLTD
topic 500
Cosmology
spellingShingle 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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