Research Papers (JVN)

Permanent URI for this collectionhttp://localhost:4000/handle/11007/400

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    Radiation backgrounds and their cosmologival implications
    (T.I.F.R., 1983-01-15) Narlikar, J. V.
    The information content of radiation backgrounds at wavelengths ranging from radio waves to gamma rays is reviewed, within the context of the standard big bang cosmology. It is shown that the various backgrounds provide useful inputs and constraints on the physical features of the universe such as the existence and growth of large scale inhomogeneities like galaxies, clusters and superclusters, the overall density of the universe, the photon to baryon ratio and the extent of antimatter in the universe, etc. It is argued that there are questions posed by the data which may require rethinking of some aspects of standard cosmology.
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    Contribution of quasistellar objects to the cosmic X-ray background
    (Indian Institute of Astrophysics, 1983-01-14) Narlikar, J. V.; Burbidge, G.
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    Empirical approach to cosmology
    (Springer, 1981-01-23) Narlikar, J. V.; Burbidge, G.
    A 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.