| dc.contributor.author | Övgün, Ali | |
| dc.date.accessioned | 2017-04-20T08:03:16Z | |
| dc.date.available | 2017-04-20T08:03:16Z | |
| dc.date.issued | 2017-02-16 | |
| dc.identifier.citation | Övgün, A. Eur. Phys. J. C (2017) 77: 105. doi:10.1140/epjc/s10052-017-4673-4 | en_US |
| dc.identifier.issn | 1434-6044 (print) | |
| dc.identifier.issn | 1434-6052 (online) | |
| dc.identifier.uri | http://dx.doi.org/10.1140/epjc/s10052-017-4673-4 | |
| dc.identifier.uri | http://hdl.handle.net/11129/3202 | |
| dc.description | The file in this item is the publisher version (published version) of the article. | en_US |
| dc.description.abstract | Despite impressive phenomenological success, cosmological models are incomplete without an understanding of what happened at the big bang singularity. Maxwell electrodynamics, considered as a source of the classical Einstein field equations, leads to the singular isotropic Friedmann solutions. In the context of Friedmann–Robertson–Walker (FRW) spacetime, we show that singular behavior does not occur for a class of nonlinear generalizations of the electromagnetic theory for strong fields. A new mathematical model is proposed for which the analytical nonsingular extension of FRW solutions is obtained by using the nonlinear magnetic monopole fields. | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | Springer | en_US |
| dc.relation.isversionof | 10.1140/epjc/s10052-017-4673-4 | en_US |
| dc.rights | info:eu-repo/semantics/openAccess | en_US |
| dc.subject | cosmology | en_US |
| dc.subject | universe | en_US |
| dc.subject | inflation | en_US |
| dc.subject | acceleration | en_US |
| dc.subject | dark energy | en_US |
| dc.subject | theoretical physics | en_US |
| dc.title | Inflation and Acceleration of the Universe by Nonlinear Magnetic Monopole Fields | en_US |
| dc.type | article | en_US |
| dc.relation.journal | The European Physical Journal C | en_US |
| dc.contributor.department | Physics Department | en_US |
| dc.identifier.volume | 77 | en_US |
| dc.identifier.issue | 105 | en_US |