2022
DOI: 10.1007/jhep05(2022)110
|View full text |Cite
|
Sign up to set email alerts
|

Gravitational instantons with conformally coupled scalar fields

Abstract: We present novel regular Euclidean solutions to General Relativity in presence of Maxwell and conformally coupled scalar fields. In particular, we consider metrics of the Eguchi-Hanson and Taub-NUT families to solve the field equations analytically. The solutions have nontrivial topology labeled by the Hirzebruch signature and Euler characteristic that we compute explicitly. We find that, although the solutions are locally inequivalent with the original (anti-)self-dual Eguchi-Hanson metric, they have the same… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
3
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
6
2

Relationship

0
8

Authors

Journals

citations
Cited by 13 publications
(3 citation statements)
references
References 125 publications
0
3
0
Order By: Relevance
“…[104,105] and the backreaction of conformally coupled scalar fields was considered in Ref. [106]. Thus, future applications of the present configuration are plausible.…”
Section: B Eguchi-hansonmentioning
confidence: 80%
“…[104,105] and the backreaction of conformally coupled scalar fields was considered in Ref. [106]. Thus, future applications of the present configuration are plausible.…”
Section: B Eguchi-hansonmentioning
confidence: 80%
“…Furthermore, the Ehlers transformations have also been used to immerse wormhole solutions into the swirling background [8]. A systematical study of composed Harrison and Ehlers transformations have also been presented recently [9].…”
Section: Introductionmentioning
confidence: 99%
“…It it known that non-minimally coupled, selfinteracting scalars with self interactions allow to construct hairy black holes as well a other interesting configurations in vacuum in GR (see e.g. [58]- [64]). Even more, quartic self interactions allow to construct hairy black holes in the presence of higher-curvature terms in dimension greater than four, ψ [65,66], which has led us to considering the 4DS-EGB model in presence of such a further scalar degree of freedom.…”
Section: Introductionmentioning
confidence: 99%