Absorber theory of radiation in expanding universe
| dc.contributor.author | Narlikar, J. V. | |
| dc.date.accessioned | 2012-03-26T13:00:31Z | |
| dc.date.available | 2012-03-26T13:00:31Z | |
| dc.date.issued | 2002-10-28 | |
| dc.description.abstract | The Wheeler-Feynman absorber theory of radiation of the symmetric combination of retarded and advanced potentials, originally developed in a static universe model, is applied to asymptotic boundary conditions for an action-at-a-distance electro dynamic framework of a Quasi-Steady State Universe; which as discussed is in opposition to the broad class of Big bang cosmologies. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/1629 | |
| dc.language.iso | en | en_US |
| dc.publisher | Kluwer Academic Publishers | en_US |
| dc.relation.ispartofseries | Gravitation and Cosmology: From the Hubble Radius to the Planck Scale, Eds. R.L. Amoroso, G. Hunter, M. Kafatos and J-P Vigier;81p., 2002 | |
| dc.subject | Wheeler-Feynman absorber theory | en_US |
| dc.subject | Symmetric combination | en_US |
| dc.subject | Universe model | en_US |
| dc.subject | Quasi-Steady State Universe | en_US |
| dc.subject | Big bang cosmologies | en_US |
| dc.title | Absorber theory of radiation in expanding universe | en_US |
| dc.type | Article | en_US |