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f(T,B) gravity in a Friedmann-Lema\^(i)tre-Robertson-Walker universe with nonzero spatial curvature
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f(T,B) gravity in a Friedmann-Lema\^(i)tre-Robertson-Walker universe with nonzero spatial curvature
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We investigate exact solutions and the asymptotic dynamics for the Friedmann-Lema\^{\i}tre-Robertson-Walker universe with nonzero spatial curvature in the fourth-order modified teleparallel gravitational theory known as $f\left( T, B\right) $ 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 Poincar\'e variables to investigate the dynamics at infinity.
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Cited by 1 Pith paper
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Degenerate and connection-dependent cosmological sectors in f(Q,C) gravity
Connection field equations force a degenerate f(R)-equivalent sector of f(Q,C) cosmology in which three geometric connections coincide, and only nonzero integration constants make the connections physically distinct.
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