Empirical approach to cosmology

dc.contributor.authorNarlikar, J. V.
dc.contributor.authorBurbidge, G.
dc.date.accessioned2012-03-18T06:33:47Z
dc.date.available2012-03-18T06:33:47Z
dc.date.issued1981-01-23
dc.description.abstractA two-component model of the universe is proposed, based on the observations of discrete extragalactic sources and the microwave background radiation. The large scale dynamics of the universe is determined by the radiation component and it leads to a characteristic size of the universe of approximately 600,000 Mpc and an age of approximately one trillion years. The second component, that of matter, occurs in discrete sources which group together in super-superclusters of characteristic size approximately 6000 Mpc and age 10 billion yr. It is suggested that the Galaxy belongs to one of these super-superclusters and that observations of discrete sources are confined to this unit. A reasonable agreement with the cosmological tests is obtained on the assumption that the geometry within a typical super-supercluster is Euclidean and that the redshifts of galaxies arise from a Doppler effect due to motions originating in a local explosion which gave birth to the super-supercluster. Further observational checks on this model are proposed.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1530
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofseriesAstrophysics and Space Sciences;Vol. 74, 1981
dc.subjectAstronomical modelsen_US
dc.subjectCosmologyen_US
dc.subjectGalactic structureen_US
dc.subjectUniverseen_US
dc.subjectBackground radiationen_US
dc.subjectMilky way galaxyen_US
dc.subjectred shiften_US
dc.subjectRelativityen_US
dc.titleEmpirical approach to cosmologyen_US
dc.typeArticleen_US

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