Under the World Tree

Einstein Summation

I often have trouble remembering the conventions for summation and which spaces the vectors are supposed to live in. I would really like to have good notes on graduate differential geometry as a whole in the future, but for now I will start with something I need to use a lot.

Definition: Let VV be a finite-dimensional (real or complex) vector space with dual VV^*. The space Vsr=VrV sV^r_{s} = V^{\otimes r} \otimes V^{* \ \otimes s} is called the space of type (r,s)-tensors. The integer rr is called the contravariant order and ss is the covariant order.

Contravariance here means that under a change of basis PBBP_{\mathcal{B} \mathcal{B'}} from basis B\mathcal{B} to B\mathcal{B'}, the coordinate vector [v1vn]B\begin{bmatrix}v_{1} \\ \vdots \\ v_{n}\end{bmatrix}_{\mathcal{B}} of any point vVv \in V , if interpreted as B\mathcal{B'} coordinates instead, gives coordinates for the point PBB1vP_{\mathcal{B} \mathcal{B'}}^{-1}v.

On the other hand, covariance says that with change-of-basis PBBP_{\mathcal{B} \mathcal{B'}} for VV, the coordinates [v1vn]B\begin{bmatrix}v^*_{1} \\ \vdots \\ v^*_{n}\end{bmatrix}_{\mathcal{B}} for vector vVv^* \in V with respect to B\mathcal{B} correspond to PBBTvP_{\mathcal{B} \mathcal{B'}}^Tv^* as coordinates for B\mathcal{B'} (since the dual transformation to left-multiplication by PBBP_{\mathcal{B} \mathcal{B'}} is given by left-multiplication by (PBB1)T(P_{\mathcal{B} \mathcal{B'}}^{-1})^T.

Physicists also like to define tensors as collections of coordinates specified by type (r,s)(r,s)-multi-indices and subject to the co/contravariance relations, which is an equivalent formulation.

For calculations, we use row vectors for coordinates in VV^* and column vectors for coordinates in VV.

Tensor contraction: For any pair of indices 1λr1 \leq \lambda \leq r, 1μs1 \leq \mu \leq s we get a homomorphism Cλμ:VsrVs1r1C_{\lambda \mu} : V^r_{s} \to V^{r-1}_{s-1}, defined by extending the map Cλμ(v1vrv 1v n)= vλ,v μv1v^λvrv 1v^ μv n\begin{aligned} &C_{\lambda \mu}(v_{1}\otimes{\dots} \otimes v_{r}\otimes v^{* \ 1}\otimes{\dots} \otimes v^{* \ n}) \\ = \ &\langle v_{\lambda}, v^{* \ \mu}\rangle v_{1}\otimes\dots \otimes \hat{v}_{\lambda} \otimes \dots \otimes v_{r}\otimes v^{* \ 1}\otimes\dots \otimes \hat{v}^{* \ \mu} \otimes \dots \otimes v^{* \ n}\end{aligned} to linearity (where ^\hat{} means to remove those indices from the tensor).

Raising and lowering indices with a (pseudo)metric: If instead of the canonical pairing between VV and VV^* we contract using an inner product with matrix ημν\eta_{\mu \nu} then we can write the front coefficient either as vλv_{\lambda}

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