We give the equations governing the shear evolution in Bianchi spacetimes for general f(R) theories of gravity. We consider the case of R n-gravity and perform a detailed analysis of the dynamics in Bianchi I cosmologies which exhibit local rotational symmetry. We find exact solutions and study their behaviour and stability in terms of the values of the parameter n. In particular, we found a set of cosmic histories in which the universe is initially isotropic, then develops shear anisotropies which approach a constant value. © 2006 IOP Publishing Ltd.
Shear dynamics in Bianchi I cosmologies with Rn-gravity
Carloni S.;
2006-01-01
Abstract
We give the equations governing the shear evolution in Bianchi spacetimes for general f(R) theories of gravity. We consider the case of R n-gravity and perform a detailed analysis of the dynamics in Bianchi I cosmologies which exhibit local rotational symmetry. We find exact solutions and study their behaviour and stability in terms of the values of the parameter n. In particular, we found a set of cosmic histories in which the universe is initially isotropic, then develops shear anisotropies which approach a constant value. © 2006 IOP Publishing Ltd.File in questo prodotto:
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