dc.creatorErices-Osorio, Cristián R.
dc.creatorRiquelme, Simón
dc.creatorZalaquett, Nicolás
dc.date2023-01-04T19:10:41Z
dc.date2023-01-04T19:10:41Z
dc.date2022
dc.date.accessioned2024-05-02T20:30:18Z
dc.date.available2024-05-02T20:30:18Z
dc.identifierhttp://repositorio.ucm.cl/handle/ucm/4338
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9274588
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 nontrivial 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.sourcePhysical Review D, 106(4), 044046
dc.titleEFT approach to black hole scalarization and its compatibility with cosmic evolution
dc.typeArticle


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