Publication
Modified Saez-Ballester scalar-tensor theory from 5D space-time
| dc.contributor.author | Rasouli, S. M. M. | |
| dc.contributor.author | Moniz, Paulo | |
| dc.date.accessioned | 2019-12-11T15:24:40Z | |
| dc.date.available | 2019-12-11T15:24:40Z | |
| dc.date.issued | 2017-12-05 | |
| dc.description.abstract | In this paper, we bring together the five-dimensional Saez-Ballester~(SB) scalar-tensor theory [1] and the induced-matter-theory~(IMT) setting [2], to obtain a modified SB theory (MSBT) in four dimensions. Specifically, by using an intrinsic dimensional reduction procedure into the SB field equations in five-dimensions, a MSBT is obtained onto a hypersurface orthogonal to the extra dimension. This four-dimensional MSBT is shown to bear distinctive new features in contrast to the usual corresponding SB theory as well as to IMT and the Modified Brans-Dicke Theory (MBDT)~\cite{RFM14}. It should be emphasized that the herein appealing solutions can emerge solely from the geometrical reductional process, from presence also of extra dimension(s) and not from any ad-hoc matter either in the bulk or on the hypersurface. Subsequently, we apply the herein MSBT to cosmology and consider an extended spatially flat FLRW geometry in a five-dimensional vacuum space-time. After obtaining the exact solutions in the bulk, we proceed to construct, by means of the MSBT setting, the corresponding dynamic, on the four-dimensional hypersurface. More precisely, we obtain the (SB) components of the induced matter, including the induced scalar potential terms. We retrieve two different classes of solutions. Concerning the first class, we show that the MSBT yields a barotropic equation of state for the induced perfect fluid. We then investigate vacuum, dust, radiation, stiff fluid and false vacuum cosmologies for this scenario and contrast the results with those obtained in the standard SB theory, IMT and BD theory. Regarding the second class solutions, we show that the scale factor behaves similar to a de Sitter (DeS) model. However, in our MSBT setting, this behavior is assisted by non-vanishing induced matter instead, without any a priori cosmological constant. | pt_PT |
| dc.description.version | info:eu-repo/semantics/publishedVersion | pt_PT |
| dc.identifier.arxiv | 712.01962v2 | |
| dc.identifier.doi | 10.1088/1361-6382/aa9ad3 | pt_PT |
| dc.identifier.uri | http://hdl.handle.net/10400.6/7714 | |
| dc.language.iso | eng | pt_PT |
| dc.peerreviewed | yes | pt_PT |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | pt_PT |
| dc.subject | Saez-Ballester scalar-tensor theory | pt_PT |
| dc.subject | Induced-matter theory | pt_PT |
| dc.subject | Extra dimensions | pt_PT |
| dc.subject | FLRW cosmology | pt_PT |
| dc.title | Modified Saez-Ballester scalar-tensor theory from 5D space-time | pt_PT |
| dc.type | journal article | |
| dspace.entity.type | Publication | |
| oaire.citation.issue | 2 | pt_PT |
| oaire.citation.startPage | 025004 | pt_PT |
| oaire.citation.title | Classical and Quantum Gravity | pt_PT |
| oaire.citation.volume | 35 | pt_PT |
| person.familyName | Mousavi Rasouli | |
| person.familyName | Moniz | |
| person.givenName | Seyed Meraj | |
| person.givenName | Paulo | |
| person.identifier | 1895963 | |
| person.identifier | 277693 | |
| person.identifier.ciencia-id | 8513-6DFF-8AE8 | |
| person.identifier.ciencia-id | B410-D0B7-55C1 | |
| person.identifier.orcid | 0000-0003-3455-1954 | |
| person.identifier.orcid | 0000-0001-7170-8952 | |
| person.identifier.rid | M-9845-2013 | |
| person.identifier.scopus-author-id | 26428481000 | |
| person.identifier.scopus-author-id | 6701832578 | |
| rcaap.rights | openAccess | pt_PT |
| rcaap.type | article | pt_PT |
| relation.isAuthorOfPublication | 48e10712-ccdc-4206-baf1-92ac569b3e46 | |
| relation.isAuthorOfPublication | 06eed88a-9063-48c2-b3b5-6bd99fad095b | |
| relation.isAuthorOfPublication.latestForDiscovery | 48e10712-ccdc-4206-baf1-92ac569b3e46 |