Interacting dark energy in f(R) gravity
Jul, 2006Citations per year
Abstract: (arXiv)
The field equations in gravity derived from the Palatini variational principle and formulated in the Einstein conformal frame yield a cosmological term which varies with time. Moreover, they break the conservation of the energy--momentum tensor for matter, generating the interaction between matter and dark energy. Unlike phenomenological models of interacting dark energy, gravity derives such an interaction from a covariant Lagrangian which is a function of a relativistically invariant quantity (the curvature scalar ). We derive the expressions for the quantities describing this interaction in terms of an arbitrary function , and examine how the simplest phenomenological models of a variable cosmological constant are related to gravity. Particularly, we show that for a flat, homogeneous and isotropic, pressureless universe. For the Lagrangian of form , which is the simplest way of introducing current cosmic acceleration in gravity, the predicted matter--dark energy interaction rate changes significantly in time, and its current value is relatively weak (on the order of 1% of ), in agreement with astronomical observations.- 95.36.+x
- 04.50.+h
- 98.80.-k
- gravitation: model
- dark energy: interaction
- field equations
- holography
- energy: density
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