Alternating Tensor Algebra

We ask for K not to have characteristic 2, for this section.

Remember that V⊗k is the space of homogeneous tensors of degree k. This is spanned by decomposable tensors $$v_1 \otimes v_2 \otimes \dots \otimes v_k,\quad v_i \in V$$
Def: The antisymmetrisation or skew-symmetrisation of decomposable tensors is defined by $$\mathcal A(v_1 \otimes \dots \otimes v_k) := \sum_{\sigma \in S_k} \text{sgn}(\sigma) v_{\sigma(1)} \otimes \dots \otimes v_{\sigma(k)}$$where the sum is taken over the symmetric group and, when the k!≠0: $$\text{Alt}(v_1 \otimes \dots\otimes v_k) := \frac1{k!} \sum_{\sigma \in S_k} \text{sgn}(\sigma) v_{\sigma(1)} \otimes \dots \otimes v_{\sigma(k)}$$
Def: In the language of tensors, a p-vector is an alternating contravariant tensor of order p. A p-vector is denoted by A[p] and characterised by $$A_{[p]} = \text{Alt}(A_{[p]}).$$The brackets here are used to indicate the alternation of the p indices set. Thus, given Ap∈V⊗p, Alt(Ap) is a p-vector. The symbols ⋀p(V) and ⋀p(V) respectively denote the space space of p-vectors and p-covectors.

Prop: Let p∈N, then $$\dim {\textstyle \bigwedge}^{!p}(V) = \dim {\textstyle \bigwedge}p(V) = {n \choose p}.$$
Cor: Let p∈N, then $$\dim {\bigwedge}p(V) = \dim {\bigwedge}(V).$$
Def: Let A[p]∈⋀p(V) be a p-vector and let B[q]∈⋀q(V) be a q vector. The exterior product ∧:⋀p(V)×⋀q(V)→⋀p+q(V) is defined by $$A
\wedge B_{[q]} := \text{Alt}(A_{[p]} \otimes B_{[q]}).$$
Prop: Let A[p]∈⋀p(V), B[q]∈⋀q(V) and C[r]∈⋀r(V), then $$(A_{[p]} \wedge B_{[q]}) \wedge C_{[r]} = A_{[p]} \wedge (B_{[q]} \wedge C_{[r]}),$$meaning that ∧ is associative.

Def: For p∈N, we can define a left action and a right action from Sp on ⋀p(V).
Let σ∈Sp, and A[p]∈⋀p(V):

Obs: We get another characterisation of ⋀p(V), it is a subspace of V⊗p such that for all A[p] either σ(A[p])=A[p] or (A[p])σ=A[p] for all σ∈Sp.

Obs: The definition of the exterior product is equivalent to $$A_{[p]} \wedge B_{[q]} := \frac{p!q!}{(p+q)!} \sum_{\sigma\in S_{p, q}} \sigma(A_{[p]} \otimes B_{[q]}), $$where Sp,q denotes the subset of Sp+q containing all σ such that σ(i)<σ(i+1) if 0<i<p, or p<i<p+q.

Prop: From this equation, it follows that u∧v=−v∧u, and v∧v=0.

Cor: A[p]∧B[q]=(−1)pqB[q]∧A[p].

Def: A p-vector that can be written as the exterior product of a p number of 1-vectors is called a simple p-vector.

Bases

Suppose that V is a finite dimensional K-vector space, and let B={e1,…,en} be a basis for V. We can construct the bases for ⋀p(V). First we need a shortcut in notation, let ⋀i∈Ivi is the exterior product of all the elements {vi∣i∈I} where I⊆{1,…,n} in the order inherited by I. With this in mind, we can define the basis of ⋀p(V) as $$\mathfrak B_p := \left{\left.\bigwedge_{i \in I} e_i; \right\rvert ; I \in [{1, \dots, n}]^p\right}$$A consequence of this basis, if A[2], then $$A_{[2]} = \frac12 \sum_{i, j = 1}^n A^{ij} e_i \wedge e_j = \sum_{1 \le i < j \le n} A^{ij} e_i \wedge e_j.$$Notice in the first expression the presence of the factor of 1/2, which is absent in the second expression. Since, in the sum ∑ij, we consider all the values for the indices i,j∈{1,…,n}, as Aij=−Aji, and as ei∧ej=−ej∧ei, we are indeed counting the same term twice.

We generalise this for ⋀p(V). An arbitrary element A[p]∈⋀p(V) can be written as $$
\begin{align*}
A_{[p]} &:= \frac{1}{p!} \sum_{\mu_1, \dots, \mu_p = 1}^n A^{\mu_1, \dots, \mu_p} e_{\mu_1} \wedge \dots \wedge e_{\mu_p} \
&= \sum_{1 \le \mu_1 <\dots < \mu_p \le n} A^{\mu_1, \dots, \mu_p} e_{\mu_1} \wedge \dots \wedge e_{\mu_p},
\end{align*}$$where, in the first case, we consider the sum over all posible values for the indices μi∈{1,…,n} for all i∈{1,…,p}, and, in the second case, we consider the sum over the indices with the restriction that μ1<μ2<⋯<μp.

Convention: In order to apply the sum convention to p-vectors as efficiently as possible, we impose the same restriction on the sum convention with respect to the indices, namely, that $$A^{\mu_1, \dots, \mu_p} e_{\mu_1} \wedge \dots \wedge e_{\mu_p} := \sum_{1 \le \mu_1 <\dots < \mu_p \le n} A^{\mu_1, \dots, \mu_p} e_{\mu_1} \wedge \dots \wedge e_{\mu_p}.$$Thus, we avoid using expressions with the factor p!.

An ordered k-tuple I=(i1,…,ik) of a positive integers is called a multi-index of length k. If I is such a multi-index and σ∈Sk is a permutation we write Iσ for the multi-index$$I = (i_{\sigma(1)},\dots, i_{\sigma(k)}).$$
We see that Iστ=(Iσ)τ for σ,τ∈Sk. We can extend the Kronecker delta notation in the following way. If I and J are multiindices of length k, we define $$\delta^I_J := \begin{cases}
\text{sgn }\sigma& \text{if neither I nor J has repeadted index and J=Iσ for some σ∈Sk }\
0 & \text{If I or J has repated index or J is not a permutation of I}.
\end

∗∗Def:∗∗Let${e1,…,en}$beabasisfor$V$and$I$beamulti−index,wedefine$$eI:=ei1∧⋯∧eik.

Obs: If J=Iσ, for some multi-indices, then eJ=(sgn σ)eI.

The significance of this that they provide a more convenient basis for ⋀p(V). We see that the set of eI is not linearly independent, because some of them are zero and the ones corresponding to different permutations of the same multi-index are constant multiples of each other. A multi-index I=(i1,…,ik) is said to be increasing if i1<⋯<ik. This means that using Einstein summation convention we can write a p-vector as $$A^I e_I := \sum_{I}' A_I e_I = \sum_{{I: 1 \le \mu_1 <\dots < \mu_p \le n}} A^{\mu_1, \dots, \mu_p} e_{\mu_1} \wedge \dots \wedge e_{\mu_p}$$and the set {eI∣I is an increasing pmulti-index} is a basis for ⋀p(V).

Def: Since ⋀n(V) is a one dimensional K-vector space, then we call the elements of ⋀n(V) are called n-vectors, and another usual denomination for n-vectors is psuedoscalars.

Def: The image Alt[T(V)] is always the alternating tensor graded subspace, it is not algebra yet since we don't have a product, denoted as A(V).

Obs: We have that the kernel of A(r) is precisely I(r), the homogeneous subset of the ideal I, the kernel of A is I.

When K has characteristic 0, there is a canonical isomorphism $$A(V) \cong {\textstyle \bigwedge}(V).$$With these isomorphisms, we see that exterior algebra of a vector space V over K can be canonically identifies with the vector subspace of T(V) that consists of antisymmetric tensors. With this isomorphism in mind, we don't need to care about ⋀p(V) as a subspace of A(V) or ⋀(V).

Cor: dim⁡⋀(V)=2n.

Def: We denote by ⟨⋅⟩p:⋀(V)→⋀p(V) as a projection from ⋀(V) to a space of p-vectors ⟨A⟩p:=A[p].

Def: We can define grade involution on ⋀p(V): $$#(A_{[p]}) = \widehat A_{[p] } := (-1)^p A_{[p]}. $$For the reversion, it follows that $$\widetilde{(v_1\wedge \dots \wedge v_p)} := v_p \wedge \dots \wedge v_1, $$this implies that A~[p]=(−1)p(p−1)/2A[p]. The conjugation of the two operations $$\overline A_{[p]} := \widetilde{\widehat A}{[p]} = \widehat{\widetilde A}.$$

Contraction, or Interior Product

Let A[p] be a p-vector and let α be a covector.

Def: The left contraction of a p-vector A[p] by a covector α, denoted from this point on by α⌋, is defined as $$(\alpha \rfloor A_{[p]})(\alpha_1, \dots, \alpha_{p-1}) := p A_{[p]}(\alpha, \alpha_1, \alpha_2, \dots, \alpha_{p-1}).$$where α1,…,αp−1 are arbitrary covectors. Taking A[p]=v1∧⋯∧vp on the right hand side of the definition means that $$(v_1\wedge \dots \wedge v_p)(\alpha, \alpha_1, \dots, \alpha_{p-1}) := \frac1{p!} \sum_{\sigma \in S_p} \text{sgn}(\sigma) \alpha(v_{\sigma(1)}) \alpha_1(v_{\sigma(2)})\dots \alpha_{p-1}(v_{\sigma(p)}).$$
This definition shows that α⌋A[p] is a (p−1)-vector.

Lemma: Let u,v∈V and α∈V′, then $$\alpha \rfloor (v \wedge u) = (\alpha \rfloor v)u - v(\alpha \rfloor u) = \alpha(v) u - v \alpha (u).$$
Prop: Let A,B∈⋀(V) and α∈V′, then $$(\alpha \rfloor A \wedge B) = (\alpha \rfloor A) \wedge B +\widehat A \wedge (\alpha \rfloor B)

∗∗Def:∗∗The∗rightcontraction∗ofa$p$−vector$A[p]$byacovector$α$,denotedfromthispointonby$⌊α$,isdefinedas$$(A[p]⌊α)(α1,…,αp−1):=pA[p](α1,α2,…,αp−1,α).

Obs: Given the definition above, let v∈V and α∈V′, then α⌋v=α(v)=v⌊α.

Prop: Let A,B∈⋀(V), and α∈V′, then $$(A \wedge B) \lfloor \alpha = A \wedge (B \lfloor \alpha ) + (A \lfloor \alpha ) \wedge\widehat B.$$
Prop: Let A∈⋀(V), and α∈V′, then $$\alpha \rfloor A = - \widehat A \lfloor \alpha.$$
We can generalise further the left and right contractions to arbitrary covectors.

Def: Given α1∧⋯∧αp, we can define $$(\alpha_1 \wedge \alpha_2 \wedge \dots \wedge \alpha_p) \rfloor := \alpha_1 \rfloor \alpha_2\rfloor\cdots \alpha_p\rfloor,$$and $$\lfloor (\alpha_1 \wedge \alpha_2 \wedge \dots \wedge \alpha_p) := \lfloor\alpha_1 \lfloor\alpha_2 \cdots \lfloor \alpha_p.$$
Obs: Using this definition of the left contraction of a 2-covector on 2-vector we get that $$(\alpha \wedge \beta)\rfloor (u \wedge v) = \alpha(v) \beta(u)- \alpha (u) \beta(v) = 2(\alpha\wedge \beta)(u \wedge v). $$This can generalised further. Let Φ[p] be a p-covector and A[p] a p-vector, then $$\Psi^{[p]} (A_{[p]}) = \frac1{p!} \Psi^{[p]}\rfloor A_{[p]}. $$
Prop: Let Ψ[p] be a p-covector and A[q] a q-vector. If p≤q, then $$\Psi^{{[p]}}\rfloor A_{[q]} = (-1)^{p(q-1)} A_{[q]} \lfloor \Psi^{[p]}.$$Similarly, if q≤p, then $$A_{[q]} \rfloor \Psi^{[p]} = (-1)^{q(p-1)} \Psi^{[p]}\lfloor A_{[q]}.$$Lastly, $$\widetilde{\Psi^{[p]}\rfloor A_{[q]}} = A_{[q]}\lfloor \Psi^{[p]}. $$

Obs: Let us note the equality $$\Psi^{[p]}\rfloor A_{[p]} = A_{[p]} \lfloor\Psi^{[p]} = A_{[p]} \rfloor \Psi^{[p]} = \Psi^{[p]} \lfloor A_{[p]}.$$

Orientation

In this section we are considering that K=R.

There is no criteria that would induce us to prefer the choice of some specific n-vector. Ia basis B:={e1,…,en} of V is taken into account, it is natural to choose the n-vector given by the exterior product of the basis vector B. No matter the order that such exterior products are taken eσ(1)∧⋯∧eσ(n) for every σ∈Sn, the result is ±e1∧⋯∧en.

Obs: Let {v1,…,vn} be n-linearly independent vectors, then v1∧⋯∧vn=Je1∧⋯∧en. where J>0 or J<0.

Def: Ω be a n-vector, then we can define two equivalence classes [Ω] and [−Ω], as $$\begin{align*}
[\Omega] &:= \left{\left. A \in { \bigwedge}_n (V);\right\rvert; \exists J >0(A =J\Omega) \right} \
[-\Omega] &:= \left{\left. A \in {\bigwedge}_n (V);\right\rvert; \exists J <0(A =J\Omega) \right}
\end{align*}.$$These two equivalence classes compromise the vector space orientation.

There exists two possible orientations for a vector space, completely determined once ab n-vector has been selected. The choice of an n-vector ΩV in an equivalence class defines a pair constituted by a vector space V endowed with an n-vector ΩV.

We can define an orientation for the dual space V′ via de n-covector ΩV∗. The question to be posed is whether the orientation of V′ can be related to the orientation of V.

Duality

If we consider the set of all alternating k-linear forms, meaning the set of alternating k-linear maps from V to the base field K. We see that the set of all alternating k-linear forms is a vector space.

By the universal property the exterior powers, the space of alternating forms of degree k on V is naturally isomorphic with the dual space (⋀k(V))∗. Lastly, if V is finite dimensional, then the latter is naturally isomorphic to ⋀k(V∗). Using the notation, from Exterior Algebra of Multicovectors, then we get that ⋀k(V)=Ak(V)≅⋀k(V∗).