Structure formation in the quasi-steady state cosmology

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dc.contributor.authorNarlikar, J. V.
dc.date.accessioned2012-03-23T13:12:34Z
dc.date.available2012-03-23T13:12:34Z
dc.date.issued2000-03-29
dc.description.abstractIn this paper we introduce a toy model for understanding the growth of structures and the two point correlation functions in the cotext of the Quasi-Steady State Cosmology (qssc). The paper first describes the essential features of the qssc and then addresses the problem of structure formation.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1563
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofseriesGeneral Relativity and Gravitation;Vol. 32, No. 6, 2000
dc.subjectTwo point correlation functionen_US
dc.subjectQuasi-Steady State Cosmology (qssc)en_US
dc.subjectBasic theory of the qsscen_US
dc.subjectMachian theory of gravityen_US
dc.subjectMatter creationen_US
dc.subjectcosmological solutionen_US
dc.subjectcosmological solutionen_US
dc.subjectGravitational perturbationsen_US
dc.titleStructure formation in the quasi-steady state cosmologyen_US
dc.typeArticleen_US

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