Finsler manifold

Let ${\displaystyle (M,a)}$ be a Riemannian manifold and b a differential one-form on M with

${\displaystyle \|b\|_{a}:={\sqrt {a^{ij}b_{i}b_{j}}}<1,}$

where ${\displaystyle (a^{ij})}$ is the inverse matrix of ${\displaystyle (a_{ij})}$ and the Einstein notation is used. Then

${\displaystyle F(x,v):={\sqrt {a_{ij}(x)v^{i}v^{j}}}+b_{i}(x)v^{i}}$

defines a Randers metric on M and ${\displaystyle (M,F)}$ is a Randers manifold, a special case of a non-reversible Finsler manifold.[1]

Let (M,d) be a quasimetric so that M is also a differentiable manifold and d is compatible with the differential structure of M in the following sense:

• Around any point z on M there exists a smooth chart (U, φ) of M and a constant C ≥ 1 such that for every x,y ∈ U

${\displaystyle {\frac {1}{C}}\|\phi (y)-\phi (x)\|\leq d(x,y)\leq C\|\phi (y)-\phi (x)\|.}$

• The function d : M × M →[0,∞] is smooth in some punctured neighborhood of the diagonal.

Then one can define a Finsler function F : TM →[0,∞] by

${\displaystyle F(x,v):=\lim _{t\to 0+}{\frac {d(\gamma (0),\gamma (t))}{t}},}$

where γ is any curve in M with γ(0) = x and γ'(0) = v. The Finsler function F obtained in this way restricts to an asymmetric (typically non-Minkowski) norm on each tangent space of M. The induced intrinsic metric d_L: M × M → [0, ∞] of the original quasimetric can be recovered from

${\displaystyle d_{L}(x,y):=\inf \left\{\ \left.\int _{0}^{1}F(\gamma (t),{\dot {\gamma }}(t))\,dt\ \right|\ \gamma \in C^{1}([0,1],M)\ ,\ \gamma (0)=x\ ,\ \gamma (1)=y\ \right\},}$

and in fact any Finsler function F : TM → [0, ∞) defines an intrinsic quasimetric d_L on M by this formula.

The Euler–Lagrange equation for the energy functional E[γ] reads in the local coordinates (x¹,...,xⁿ,v¹,...,vⁿ) of TM as

${\displaystyle g_{ik}{\Big (}\gamma (t),{\dot {\gamma }}(t){\Big )}{\ddot {\gamma }}^{i}(t)+\left({\frac {\partial g_{ik}}{\partial x^{j}}}{\Big (}\gamma (t),{\dot {\gamma }}(t){\Big )}-{\frac {1}{2}}{\frac {\partial g_{ij}}{\partial x^{k}}}{\Big (}\gamma (t),{\dot {\gamma }}(t){\Big )}\right){\dot {\gamma }}^{i}(t){\dot {\gamma }}^{j}(t)=0,}$

where k=1,...,n and g_ij is the coordinate representation of the fundamental tensor, defined as

${\displaystyle g_{ij}(x,v):=g_{v}\left({\tfrac {\partial }{\partial x^{i}}}{\big |}_{x},{\tfrac {\partial }{\partial x^{j}}}{\big |}_{x}\right).}$

Assuming the strong convexity of F²(x,v) with respect to v∈T_xM, the matrix g_ij(x,v) is invertible and its inverse is denoted by g^ij(x,v). Then γ:[a,b]→M is a geodesic of (M,F) if and only if its tangent curve γ':[a,b]→TM \0 is an integral curve of the smooth vector field H on TM \0 locally defined by

${\displaystyle H|_{(x,v)}:=v^{i}{\tfrac {\partial }{\partial x^{i}}}{\big |}_{(x,v)}-\ 2G^{i}(x,v){\tfrac {\partial }{\partial v^{i}}}{\big |}_{(x,v)},}$

where the local spray coefficients Gⁱ are given by

${\displaystyle G^{i}(x,v):={\frac {g^{ij}(x,v)}{4}}\left(2{\frac {\partial g_{jk}}{\partial x^{\ell }}}(x,v)-{\frac {\partial g_{k\ell }}{\partial x^{j}}}(x,v)\right)v^{k}v^{\ell }.}$

The vector field H on TM/0 satisfies JH = V and [V,H] = H, where J and V are the canonical endomorphism and the canonical vector field on TM \0. Hence, by definition, H is a spray on M. The spray H defines a nonlinear connection on the fibre bundle TM \0 → M through the vertical projection

${\displaystyle v:T(TM\setminus 0)\to T(TM\setminus 0)\quad$ ;\quad v:={\tfrac {1}{2}}{\big (}I+{\mathcal {L}}_{H}J{\big )}.}

In analogy with the Riemannian case, there is a version

${\displaystyle D_{\dot {\gamma }}D_{\dot {\gamma }}X(t)+R_{\dot {\gamma }}({\dot {\gamma }}(t),X(t))=0}$

of the Jacobi equation for a general spray structure (M,H) in terms of the Ehresmann curvature and nonlinear covariant derivative.

By Hopf–Rinow theorem there always exist length minimizing curves (at least in small enough neighborhoods) on (M, F). Length minimizing curves can always be positively reparametrized to be geodesics, and any geodesic must satisfy the Euler–Lagrange equation for E[γ]. Assuming the strong convexity of F² there exists a unique maximal geodesic γ with γ(0) = x and γ'(0) = v for any (x, v) ∈ TM \ 0 by the uniqueness of integral curves.

If F² is strongly convex, geodesics γ : [0, b] → M are length-minimizing among nearby curves until the first point γ(s) conjugate to γ(0) along γ, and for t > s there always exist shorter curves from γ(0) to γ(t) near γ, as in the Riemannian case.