I) In Palatini $f(R)$ gravity, the Lagrangian density is
$$ {\cal L}~=~ \sqrt{-g} f(R), $$
with $$R~:=~ g^{\mu\nu} R_{\mu\nu}(\Gamma),$$
and where $\Gamma^{\lambda}_{\mu\nu}=\Gamma^{\lambda}_{\nu\mu}$ is an arbitrary torsionfree$^1$ connection.
II) As OP mentions, the word Palatini refers to that the metric $g_{\mu\nu}$ and the connection $\Gamma^{\lambda}_{\mu\nu}$ are independent variables. We therefore get two types of EL equations:
The EL equations for the metric $g_{\mu\nu}$ are the generalization of EFE.
The EL equations for the connection $\Gamma^{\lambda}_{\mu\nu}$ turns out to be the metric compatibility condition for a second metric defined as
$$ \hat{g}_{\mu\nu}~:=~f^{\prime}(R) g_{\mu\nu}. $$
In other words, the classical solution for $\Gamma^{\lambda}_{\mu\nu}$ is the Levi-Civita connection for the second metric $\hat{g}_{\mu\nu}$.
III) So Einstein gravity (GR) with a possible cosmological constant
$$ f(R)~=~R-2\Lambda, $$
or equivalently
$$ f^{\prime}(R)~=~1,$$
corresponds to the special case where the two metrics $g_{\mu\nu}$ and $\hat{g}_{\mu\nu}$ coincide, and hence $\Gamma^{\lambda}_{\mu\nu}$ becomes the Levi-Civita connection for $g_{\mu\nu}$.
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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