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   <dc:title>Properties of expanding universes</dc:title>
   <dc:identifier xsi:type="dcterms:DOI">10.17863/CAM.11283</dc:identifier>
   <dc:creator>Hawking, Stephen W</dc:creator>
   <uketdterms:authoridentifier xsi:type="uketdterms:ORCID">000000029079593X</uketdterms:authoridentifier>
   <uketdterms:advisor>Sciama, D</uketdterms:advisor>
   <dcterms:abstract>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.</dcterms:abstract>
   <uketdterms:institution>University of Cambridge</uketdterms:institution>
   <dcterms:issued>1966-03-15</dcterms:issued>
   <dc:type>Thesis</dc:type>
   <uketdterms:qualificationlevel>Doctoral</uketdterms:qualificationlevel>
   <uketdterms:qualificationname>Doctor of Philosophy (PhD)</uketdterms:qualificationname>
   <dc:language>eng</dc:language>
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   <dc:subject>gravity</dc:subject>
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