I) In Palatini f(R) gravity, the Lagrangian density is
L = √−gf(R),
with R := gμνRμν(Γ),
and where Γλμν=Γλνμ is an arbitrary torsionfree1 connection.
II) As OP mentions, the word Palatini refers to that the metric gμν and the connection Γλμν are independent variables. We therefore get two types of EL equations:
The EL equations for the metric gμν are the generalization of EFE.
The EL equations for the connection Γλμν turns out to be the metric compatibility condition for a second metric defined as
ˆgμν := f′(R)gμν.
In other words, the classical solution for Γλμν is the Levi-Civita connection for the second metric ˆgμν.
III) So Einstein gravity (GR) with a possible cosmological constant
f(R) = R−2Λ,
or equivalently
f′(R) = 1,
corresponds to the special case where the two metrics gμν and ˆgμν coincide, and hence Γλμν becomes the Levi-Civita connection for gμν.
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1 One could allow a non-dynamical torsion piece, but we will not pursuit this here for simplicity. For more on torsion, see e.g. also this Phys.SE post.
This post imported from StackExchange Physics at 2014-10-23 07:31 (UTC), posted by SE-user Qmechanic