dc.creatorErices-Osorio, Cristián R.
dc.creatorRiquelme, Simón
dc.creatorZalaquett, Nicolás
dc.date2023-09-04T12:45:00Z
dc.date2023-09-04T12:45:00Z
dc.date2023
dc.date.accessioned2024-05-02T20:31:37Z
dc.date.available2024-05-02T20:31:37Z
dc.identifierhttp://repositorio.ucm.cl/handle/ucm/4954
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9275175
dc.descriptionWe address the issue of black hole scalarization and its compatibility with cosmic inflation and Big Bang cosmology from an effective field theory (EFT) point of view. In practice, using a well-defined and healthy toy model which (in part) has been broadly considered in the literature, we consider how higher-order theories of gravity, up to cubic operators in Riemann curvature, fit within this context. Interestingly enough, we find that already at this minimal level, there is a non-trivial interplay between the Wilson coefficients which are otherwise completely independent, constraining the parameter space where scalarization may actually occur.Conclusively, we claim that the EFT does exhibit black hole scalarization, remaining compatible with the inflationary paradigm, and admitting General Relativity as a cosmological attractor.
dc.languageen
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.sourceActa Physica Polonica B, Proceedings Supplement, 16(6), 6-A15
dc.titleEft approach to black hole scalarization and its compatibility with cosmic evolution
dc.typeArticle


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