Bianchi type I expanding universe in Weyl-invariant gravity with a quartic interaction term

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DC 欄位	值	語言
dc.contributor.author	Kao, W. F.	en_US
dc.contributor.author	Lin, Ing-Chen	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.identifier.issn	1434-6044	en_US
dc.identifier.uri	http://dx.doi.org/10.1140/epjc/s10052-017-5387-3	en_US
dc.identifier.uri	http://hdl.handle.net/11536/144136	-
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.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
dc.identifier.doi	10.1140/epjc/s10052-017-5387-3	en_US
dc.identifier.journal	EUROPEAN PHYSICAL JOURNAL C	en_US
dc.citation.volume	77	en_US
dc.citation.issue	11	en_US
dc.citation.spage	0	en_US
dc.citation.epage	0	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000416369600001	en_US
dc.citation.woscount	0	en_US
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