# Density on a manifold

In mathematics, and specifically differential geometry, a density is a spatially varying quantity on a differentiable manifold that can be integrated in an intrinsic manner. Abstractly, a density is a section of a certain line bundle, called the density bundle. An element of the density bundle at x is a function that assigns a volume for the parallelotope spanned by the n given tangent vectors at x.
From the operational point of view, a density is a collection of functions on coordinate charts which become multiplied by the absolute value of the Jacobian determinant in the change of coordinates. Densities can be generalized into s-densities, whose coordinate representations become multiplied by the s-th power of the absolute value of the jacobian determinant. On an oriented manifold, 1-densities can be canonically identified with the n-forms on M. On non-orientable manifolds this identification cannot be made, since the density bundle is the tensor product of the orientation bundle of M and the n-th exterior product bundle of T$^∗$M (see pseudotensor).

## Motivation (densities in vector spaces)

In general, there does not exist a natural concept of a "volume" for a parallelotope generated by vectors v$_1$, ..., v$_n$ in a n-dimensional vector space V. However, if one wishes to define a function μ : V × ... × V → R that assigns a volume for any such parallelotope, it should satisfy the following properties:
* If any of the vectors v$_k$ is multiplied by λ ∈ R, the volume should be multiplied by |λ|.
* If any linear combination of the vectors v$_1$, ..., v$_{j−1}$, v$_{j+1}$, ..., v$_n$ is added to the vector v$_j$, the volume should stay invariant.
These conditions are equivalent to the statement that μ is given by a translation-invariant measure on V, and they can be rephrased as
    $\mu (Av_{1},\ldots ,Av_{n})=\left|\det A\right|\mu (v_{1},\ldots ,v_{n}),\quad A\in \operatorname {GL} (V).$
Any such mapping μ : V × ... × V → R is called a density on the vector space V. Note that if (v$_1$, ..., v$_n$) is any basis for V, then fixing μ(v$_1$, ..., v$_n$) will fix μ entirely; it follows that the set Vol(V) of all densities on V forms a one-dimensional vector space. Any n-form ω on V defines a density |ω| on V by
    $|\omega |(v_{1},\ldots ,v_{n}):=|\omega (v_{1},\ldots ,v_{n})|.$

### Orientations on a vector space

The set Or(V) of all functions o : V × ... × V → R that satisfy
    $o(Av_{1},\ldots ,Av_{n})=\operatorname {sign} (\det A)o(v_{1},\ldots ,v_{n}),\quad A\in \operatorname {GL} (V)$
if $v_{1},\ldots ,v_{n}$ are linearly independent and $o(v_{1},\ldots ,v_{n})=0$ otherwise
forms a one-dimensional vector space, and an orientation on V is one of the two elements o ∈ Or(V) such that |o(v$_1$, ..., v$_n$)| = 1 for any linearly independent v$_1$, ..., v$_n$. Any non-zero n-form ω on V defines an orientation o ∈ Or(V) such that
    $o(v_{1},\ldots ,v_{n})|\omega |(v_{1},\ldots ,v_{n})=\omega (v_{1},\ldots ,v_{n}),$
and vice versa, any o ∈ Or(V) and any density μ ∈ Vol(V) define an n-form ω on V by
    $\omega (v_{1},\ldots ,v_{n})=o(v_{1},\ldots ,v_{n})\mu (v_{1},\ldots ,v_{n}).$
In terms of tensor product spaces,
    $\operatorname {Or} (V)\otimes \operatorname {Vol} (V)=\bigwedge ^{n}V^{*},\quad \operatorname {Vol} (V)=\operatorname {Or} (V)\otimes \bigwedge ^{n}V^{*}.$

### s-densities on a vector space

The s-densities on V are functions μ : V × ... × V → R such that
    $\mu (Av_{1},\ldots ,Av_{n})=\left|\det A\right|^{s}\mu (v_{1},\ldots ,v_{n}),\quad A\in \operatorname {GL} (V).$
Just like densities, s-densities form a one-dimensional vector space Vol$^s$(V), and any n-form ω on V defines an s-density |ω|$^s$ on V by
    $|\omega |^{s}(v_{1},\ldots ,v_{n}):=|\omega (v_{1},\ldots ,v_{n})|^{s}.$
The product of s$_1$- and s$_2$-densities μ$_1$ and μ$_2$ form an (s$_1$+s$_2$)-density μ by
    $\mu (v_{1},\ldots ,v_{n}):=\mu _{1}(v_{1},\ldots ,v_{n})\mu _{2}(v_{1},\ldots ,v_{n}).$
In terms of tensor product spaces this fact can be stated as
    $\operatorname {Vol} ^{s_{1}}(V)\otimes \operatorname {Vol} ^{s_{2}}(V)=\operatorname {Vol} ^{s_{1}+s_{2}}(V).$

## Definition

Formally, the s-density bundle Vol$^s$(M) of a differentiable manifold M is obtained by an associated bundle construction, intertwining the one-dimensional group representation
    $\rho (A)=\left|\det A\right|^{-s},\quad A\in \operatorname {GL} (n)$
of the general linear group with the frame bundle of M.
The resulting line bundle is known as the bundle of s-densities, and is denoted by
    $\left|\Lambda \right|_{M}^{s}=\left|\Lambda \right|^{s}(TM).$
A 1-density is also referred to simply as a density.
More generally, the associated bundle construction also allows densities to be constructed from any vector bundle E on M.
In detail, if (U$_α$,φ$_α$) is an atlas of coordinate charts on M, then there is associated a local trivialization of $\left|\Lambda \right|_{M}^{s}$
    $t_{\alpha }:\left|\Lambda \right|_{M}^{s}|_{U_{\alpha }}\to \phi _{\alpha }(U_{\alpha })\times \mathbb {R}$
subordinate to the open cover U$_α$ such that the associated GL(1)-cocycle satisfies
    $t_{\alpha \beta }=\left|\det(d\phi _{\alpha }\circ d\phi _{\beta }^{-1})\right|^{-s}.$

## Integration

Densities play a significant role in the theory of integration on manifolds. Indeed, the definition of a density is motivated by how a measure dx changes under a change of coordinates (Folland 1999, Section 11.4, pp. 361-362).
Given a 1-density ƒ supported in a coordinate chart U$_α$, the integral is defined by
    $\int _{U_{\alpha }}f=\int _{\phi _{\alpha }(U_{\alpha })}t_{\alpha }\circ f\circ \phi _{\alpha }^{-1}d\mu$
where the latter integral is with respect to the Lebesgue measure on R$^n$. The transformation law for 1-densities together with the Jacobian change of variables ensures compatibility on the overlaps of different coordinate charts, and so the integral of a general compactly supported 1-density can be defined by a partition of unity argument. Thus 1-densities are a generalization of the notion of a volume form that does not necessarily require the manifold to be oriented or even orientable. One can more generally develop a general theory of Radon measures as distributional sections of $|\Lambda |_{M}^{1}$ using the Riesz-Markov-Kakutani representation theorem.
The set of 1/p-densities such that $|\phi |_{p}=\left(\int |\phi |^{p}\right)^{1/p}<\infty$ is a normed linear space whose completion $L^{p}(M)$ is called the intrinsic L$^p$ space of M.

## Conventions

In some areas, particularly conformal geometry, a different weighting convention is used: the bundle of s-densities is instead associated with the character
    $\rho (A)=\left|\det A\right|^{-s/n}.$
With this convention, for instance, one integrates n-densities (rather than 1-densities). Also in these conventions, a conformal metric is identified with a tensor density of weight 2.

## Properties

* The dual vector bundle of $|\Lambda |_{M}^{s}$ is $|\Lambda |_{M}^{-s}$.
* Tensor densities are sections of the tensor product of a density bundle with a tensor bundle.