Stability of cosmic structures in scalar–tensor theories of gravity

Grigoris Panotopoulos, Ángel Rincón

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

12 Citas (Scopus)

Resumen

In the present work we study a concrete model of scalar–tensor theory of gravity characterized by two free parameters, and we compare its predictions to observational data and constraints coming from supernovae, solar system tests and the stability of cosmic structures. First an exact analytical solution at the background level is obtained. Using that solution the expression for the turnaround radius is computed. Finally we show graphically how current data and limits put bounds on the parameters of the model at hand.

Idioma originalInglés
Número de artículo40
PublicaciónEuropean Physical Journal C
Volumen78
N.º1
DOI
EstadoPublicada - 1 ene. 2018
Publicado de forma externa

Huella

Profundice en los temas de investigación de 'Stability of cosmic structures in scalar–tensor theories of gravity'. En conjunto forman una huella única.

Citar esto