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 |