Bianchi type I expanding universe in Weyl-invariant gravity with a quartic interaction term
| dc.citation.epage | 0 | en_US |
| dc.citation.issue | 11 | en_US |
| dc.citation.spage | 0 | en_US |
| dc.citation.volume | 77 | en_US |
| dc.citation.woscount | 0 | en_US |
| dc.contributor.author | Kao, W. F. | en_US |
| dc.contributor.author | Lin, Ing-Chen | en_US |
| dc.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | en_US |
| dc.date.accessioned | 2019-04-03T06:41:20Z | |
| dc.date.available | 2019-04-03T06:41:20Z | |
| dc.date.issued | 2017-11-26 | en_US |
| dc.description.abstract | We will focus on the effect of a Weyl-invariant model with a quadratic interaction term and a free scalar field psi. A set of analytic solutions will be obtained for this model. This model provides a dynamical alternative to the standard Lambda CDM model. In particular, we will show that the quartic Weyl-invariant model prediction is consistent with the Hubble diagram observations. | en_US |
| dc.identifier.doi | 10.1140/epjc/s10052-017-5387-3 | en_US |
| dc.identifier.issn | 1434-6044 | en_US |
| dc.identifier.journal | EUROPEAN PHYSICAL JOURNAL C | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1140/epjc/s10052-017-5387-3 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/144136 | |
| dc.identifier.wosnumber | WOS:000416369600001 | en_US |
| dc.language.iso | en_US | en_US |
| dc.title | Bianchi type I expanding universe in Weyl-invariant gravity with a quartic interaction term | en_US |
| dc.type | Article | en_US |