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dc.contributor.authorBuers, Awour
dc.date.accessioned2013-06-03T11:31:59Z
dc.date.available2013-06-03T11:31:59Z
dc.date.issued1998
dc.identifier.citationA Composite Spacetime Curvature Model, BUERS, DR. AWUOR JOHN, and OTIENO PROF. MALO J. , Mod Phys. Lett. A, Vol 13, No 9 (1998)677 - 683., (1998) copy at http://profiles.uonbi.ac.ke/buers/publications/composite-spacetime-curvature-modelen
dc.identifier.urihttp://www.worldscientific.com/doi/abs/10.1142/S0217732398000735
dc.identifier.urihttp://erepository.uonbi.ac.ke:8080/xmlui/handle/123456789/28709
dc.description.abstractWe develop a curvature specification scheme in which the constraint effects of a localized gravitational potential source on the Hubble expansion comprises the characteristics of the large scale dynamics of the entire universe. Our result is a composite curvature model which has a dynamical Euclidean horizon (of zero curvature) that provides an alternative to the event horizon in the determination of the local scale evolution of space–time. Read More: http://www.worldscientific.com/doi/abs/10.1142/S0217732398000735
dc.language.isoenen
dc.titleA Composite Spacetime Curvature Modelen
dc.typeArticleen
local.publisherDepartment of Physics, University of Nairobi.en


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