f(T,B) gravity in a Friedmann–Lemaître–Robertson–Walker universe with nonzero spatial curvature

Paliathanasis; A.; León; G.

Keywords: closed universe; modified gravity; open universe; teleparallel cosmology

Abstract

We investigate exact solutions and the asymptotic dynamics for the Friedmann–Lemaître–Robertson–Walker universe with nonzero spatial curvature in the fourth-order modified teleparallel gravitational theory known as (Formula presented.) theory. We show that the field equations admit a minisuperspace description, and they can reproduce any exact form of the scale factor. Moreover, we calculate the equilibrium points and analyze their stability. We show that Milne and Milne-like solutions are supported, and the de Sitter universe is provided. To complete our analysis, we use Poincaré variables to investigate the dynamics at infinity. © 2022 The Authors. Mathematical Methods in the Applied Sciences published by John Wiley & Sons, Ltd.

Más información

Título según WOS: f(T,B)$$ oldsymbol{f}left(oldsymbol{T},oldsymbol{B} ight) $$ gravity in a Friedmann-Lemaitre-Robertson-Walker universe with nonzero spatial curvature
Título según SCOPUS: f(T,B) gravity in a Friedmann–Lemaître–Robertson–Walker universe with nonzero spatial curvature
Título de la Revista: Mathematical Methods in the Applied Sciences
Volumen: 46
Número: 4
Editorial: John Wiley and Sons Ltd
Fecha de publicación: 2023
Página de inicio: 3905
Página final: 3922
Idioma: English
DOI:

10.1002/mma.8728

Notas: ISI, SCOPUS