Title:
Bounce conditions in Kantowski-Sachs and Bianchi cosmologies in modified gravity theories

dc.contributor.authorT. Singh
dc.contributor.authorR. Chaubey
dc.contributor.authorAshutosh Singh
dc.date.accessioned2026-02-07T06:11:06Z
dc.date.issued2015
dc.description.abstractMany cosmological scenarios envisage either a bounce of the universe at early times, or a collapse locally to form a black hole which re-expands into a new expanding universe region. Energy conditions preclude this phenomena for ordinary matter in general relativistic universe, but scalar or other types of fields can violate some of these conditions, and so can, possibly, provide conditions for a bouncing universe. In this paper, we have investigated the necessary conditions for a bounce in Kantowski-Sachs (KS) and Bianchi type models in some modified theories of gravity like Hoyle-Narlikar creation field theory, Lyra geometry, general class of scalar-tensor theories, Einstein's theory with variable cosmological term. © 2015 World Scientific Publishing Company.
dc.identifier.doi10.1142/S0217751X15500736
dc.identifier.issn0217751X
dc.identifier.urihttps://doi.org/10.1142/S0217751X15500736
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/27786
dc.publisherWorld Scientific Publishing Co. Pte Ltd
dc.subjectBounce
dc.subjectCosmological model
dc.subjectModified gravity
dc.titleBounce conditions in Kantowski-Sachs and Bianchi cosmologies in modified gravity theories
dc.typePublication
dspace.entity.typeArticle

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