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dc.contributor.author | Odintsov S.D. | |
dc.contributor.author | Oikonomou V.K. | |
dc.date.accessioned | 2021-02-25T20:35:04Z | |
dc.date.available | 2021-02-25T20:35:04Z | |
dc.date.issued | 2020 | |
dc.identifier.issn | 0370-2693 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/161860 | |
dc.description.abstract | © 2020 The Authors We revisit the Einstein-Gauss-Bonnet theory in view of the GW170817 event, which compels that the gravitational wave speed is equal to cT2=1 in natural units. We use an alternative approach compared to one previous work of ours, which enables us to express all the slow-roll indices and the observational indices as functions of the scalar field. Using our formalism we investigate if the Swampland criteria are satisfied for the Einstein-Gauss-Bonnet theory and as we demonstrate, the Swampland criteria are satisfied for quite general forms of the potential and the Gauss-Bonnet coupling function ξ(ϕ), if the slow-roll conditions are assumed to hold true. | |
dc.relation.ispartofseries | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | |
dc.title | Swampland implications of GW170817-compatible Einstein-Gauss-Bonnet gravity | |
dc.type | Article | |
dc.relation.ispartofseries-volume | 805 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS03702693-2020-805-SID85083584371 |