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 |
|