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dc.contributor.authorDESHPANDE, KAUSTUBH SUDHIRen_US
dc.date.accessioned2020-10-20T07:07:33Z-
dc.date.available2020-10-20T07:07:33Z-
dc.date.issued2014-09en_US
dc.identifier.citationPramana, 83, 449–456.en_US
dc.identifier.issn0304-4289en_US
dc.identifier.issn0973-7111en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5225-
dc.identifier.urihttps://doi.org/10.1007/s12043-014-0777-7en_US
dc.description.abstractAction-at-a-distance electrodynamics – alternative approach to field theory – can be extended to cosmological models using conformal symmetry. An advantage of this is that, the origin of arrow of time in electromagnetism can be attributed to the cosmological structure. Different cosmological models can be investigated, based on Wheeler–Feynman absorber theory, and only those models can be considered viable for our Universe which have net full retarded electromagnetic interactions, i.e., forward direction of time. This work evaluates the quasi-steady-state model and demonstrates that it admits full retarded and not advanced solution. Thus, quasi-steady-state cosmology (QSSC) satisfies this necessary condition for a correct cosmological model, based on action-at-a-distance formulation.en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.subjectAction-at-a-distance electrodynamicsen_US
dc.subjectQuasi-steady-state cosmologyen_US
dc.subjectRetarded and advanced interactionsen_US
dc.subjectWheeler-Feynman absorber theoryen_US
dc.subject2014en_US
dc.titleAction-at-a-distance electrodynamics in quasi-steady-state cosmologyen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePramanaen_US
dc.publication.originofpublisherIndianen_US
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