Quasi-steady state cosmology

dc.contributor.authorHoyle, F.
dc.contributor.authorBurbidge, G.
dc.contributor.authorNarlikar, J. V.
dc.date.accessioned2012-03-11T15:11:13Z
dc.date.available2012-03-11T15:11:13Z
dc.date.issued1995-03-14
dc.description.abstractBecause of a number of unsatisfactory features of the standard hot big bang cosmology, it is argued that there is a case for exploring alternative approaches to cosmology. The approach described here called the quasi steady state cosmology (QSSC, uses a field theoretic description of matter creation within the framework of general relativity. A cosmological solutions with the universe expanding exponentially along with cycles of expansion and contraction arises from mini-creation events taking place near the event horizons of highly collapsed massive objects. The now familiar phenomena like QSOs, AGN, radio sources etc. are the manifestations of matter creation in such events. In this way cosmology is seen to be related to high energy astrophysics in a very direct way. The quasi can explain the abundances of light nuclei and the microwave background, observed large scale features of the universe like the m-z relation, the source count, the angular size-redshift relation, as well as observed distribution of the ages of galaxies.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1141
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.ispartofseriesJournal of Astrophysics and Astronomy Supplement;Vol. 16, 1995
dc.subjectCosmological modelsen_US
dc.subjectCreation of matteren_US
dc.subjectSteady state cosmologyen_US
dc.subjectOrigin of Nucleien_US
dc.subjectMicrowave backgrounden_US
dc.subjectCosmology and Astrophysicsen_US
dc.titleQuasi-steady state cosmologyen_US
dc.typeArticleen_US

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