Publication:
Instability of some k -essence spacetimes

dc.contributor.authorRodrigues, D. C.
dc.contributor.authorBronnikov, K. A.
dc.contributor.authorFabris, J. C.
dc.contributor.authorБронников, Кирилл Александрович
dc.date.accessioned2024-11-25T15:35:34Z
dc.date.available2024-11-25T15:35:34Z
dc.date.issued2020
dc.description.abstract© 2020 World Scientific Publishing Company.We study the stability properties of static, spherically symmetric configurations in k-essence theories with the Lagrangians of the form F(X), X φ,αφ,α. The instability under spherically symmetric perturbations is proved for the two recently obtained exact solutions for F(X) = F0X1/3 and for F(X) = F0X1/2 - 2Λ, where F0 and Λare constants. The first solution describes a black hole in an asymptotically singular spacetime, the second one contains two horizons of infinite area connected by a wormhole. It is argued that spherically symmetric k-essence configurations with n < 1/2 are generically unstable because the perturbation equation is not of hyperbolic type.
dc.identifier.citationRodrigues, D. C. Instability of some k -essence spacetimes / Rodrigues, D.C., Bronnikov, K.A., Fabris, J.C. // International Journal of Modern Physics D. - 2020. - 10.1142/S0218271820500169
dc.identifier.doi10.1142/S0218271820500169
dc.identifier.urihttps://www.doi.org/10.1142/S0218271820500169
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dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/20141
dc.relation.ispartofInternational Journal of Modern Physics D
dc.titleInstability of some k -essence spacetimes
dc.typeArticle
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