At the beginning of the paper "The curvature of 4-dimensional Einstein spaces", by Singer and Thorpe, the authors define the space $\mathcal{R}$ of curvature tensors of the vector space $V$ as the set of symmetric bilinear transformations on the space of bivectors $\Lambda^{2}(V).$
Few lines after this, they define the ''Bianchi map'' $b$ as an operator $b : \mathcal{R} \rightarrow \mathcal{R}$ in the following way: $$[b(R)](u_{1},u_{2})u_{3}=\sum_{\sigma \in S_{n}} R(u_{\sigma(1)},u_{\sigma(2)})u_{\sigma(3)},$$ but they do not explain the notation. If $R$ is a transformation $$R: \Lambda^{2}(V) \rightarrow \Lambda^{2}(V),$$ and $u_{1},u_{2}$ and $u_{3}$ are, I presume,vectors of $V,$ what is the meaning of $R(u_{\sigma(1)},u_{\sigma(2)})u_{\sigma(3)}$?
Also, they define immediately after this the ''Ricci contraction'' $r$ as an operator from $\mathcal{R}$ to the space of symmetric linear transformations of $V$ by means of: $$\langle r(R)(v),w \rangle=\mathrm{Tr}\{u \rightarrow R(v,u)w \}.$$
I see that this strongly resembles to the Ricci tensor that one usually meets in riemannian geometry, but I have a similar notational problem with this last definition.
If someone could possible clarify the notation and explain a little this way to look at the curvature tensor (or give me some references) I would be really grateful.
Well, Singer and Thorpe do explain the notation (see p.356 in the original text) by saying that
So the meaning of $R(x,y)z$ is an endomorphism $R(x,y)$ applied to an element $z$.
By the "usual isomorphisms" they mean "the musical isomorphisms", that is the identification of the tangent and cotangent space.
In the abstract index notation this can be explained as viewing a tensor with symmetries $$ R_{abcd} = R_{[ab][cd]}=R_{[cd][ab]} $$ as equivalent (up to raising an index) to a tensor $R_{ab}{}^c{}_d = R_{[ab]}{}^c{}_d$, and $(R(x,y)z)^c = x^a y^b R_{a b}{}^c{}_d z^d$.