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In [[mathematics]], particularly [[differential geometry]], a '''Finsler manifold''' is a [[differentiable manifold]] together with the structure of an [[intrinsic equation|intrinsic]] [[quasimetric space#Quasimetrics|quasimetric space]] in which the length of any [[rectifiable curve]] {{nowrap|''γ'' : [''a'',''b''] → ''M''}} is given by the length [[functional (mathematics)|functional]]
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:<math>L[\gamma] = \int_a^b F(\gamma(t),\dot{\gamma}(t))\,dt,</math>
 
where ''F''(''x'',&nbsp;·&nbsp;) is a '''Minkowski norm''' (or at least an [[asymmetric norm]]) on each [[tangent space]] ''T''<sub>''x''</sub>''M''. Finsler manifolds non-trivially generalize [[Riemannian manifold]]s in the sense that they are not necessarily infinitesimally [[Euclidean space|Euclidean]]. This means that the (asymmetric) norm on each tangent space is not necessarily induced by an [[inner product]] ([[metric tensor]]).
 
{{harvs|txt|authorlink=Élie  Cartan|last=Cartan|first=Élie|year1=1933}} named Finsler manifolds after [[Paul Finsler]], who studied this geometry in his dissertation {{harv|Finsler|1918}}.
 
==Definition==
A '''Finsler manifold''' is a [[differentiable manifold]] ''M'' together with a '''Finsler function''' ''F'' defined on the [[tangent bundle]] of ''M'' so that for all tangent vectors ''v'',
 
* ''F'' is [[smooth function|smooth]] on the complement of the zero section of ''TM''.
* ''F''(''v'')&nbsp;≥&nbsp;0 with equality if and only if ''v''&nbsp;=&nbsp;0 ([[positive-definite function|positive definiteness]]).
* ''F''(λ''v'')&nbsp;=&nbsp;λ''F''(''v'') for all λ&nbsp;≥&nbsp;0 (but not necessarily for&nbsp;λ&nbsp;<&nbsp;0)  ([[homogeneous function|homogeneity]]).
* ''F''(''v''&nbsp;+&nbsp;''w'')&nbsp;≤&nbsp;''F''(''v'')&nbsp;+&nbsp;''F''(''w'') for all ''w'' at the same tangent space with ''v'' ([[subadditivity]]).
 
In other words, ''F'' is an [[asymmetric norm]] on each tangent space. Typically one replaces the subadditivity with the following strong convexity condition:
 
* For each tangent vector ''v'', the [[Hessian matrix|hessian]] of ''F''<sup>2</sup> at ''v'' is [[Positive-definite matrix|positive definite]].
 
Here the hessian of ''F''<sup>2</sup> at ''v'' is the [[symmetric tensor|symmetric]] [[bilinear form]]
 
:<math>\mathbf{g}_v(X,Y) := \frac{1}{2}\left.\frac{\partial^2}{\partial s\partial t}\left[F(v + sX + tY)^2\right]\right|_{s=t=0},</math>
 
also known as the '''fundamental tensor''' of ''F'' at ''v''. Strong convexity of ''F''<sup>2</sup> implies the subadditivity with a strict inequality if ''u''/''F''(''u'')&nbsp;≠&nbsp;''v''/''F''(''v''). If ''F''<sup>2</sup> is strongly convex, then ''F'' is a '''Minkowski norm''' on each tangent space.
 
A Finsler metric is '''reversible''' if, in addition,
 
* ''F''(&minus;''v'')&nbsp;=&nbsp;''F''(''v'') for all tangent vectors ''v''.
 
A reversible Finsler metric defines a [[norm (mathematics)|norm]] (in the usual sense) on each tangent space.
 
==Examples==
* [[Normed vector space]]s of finite dimension, such as [[Euclidean space]]s, whose norms are smooth outside the origin.
* [[Riemannian manifold]]s (but not [[pseudo-Riemannian manifold]]s) are special cases of Finsler manifolds.
 
===Randers manifolds===
Let (''M'',''a'') be a [[Riemannian manifold]] and ''b'' a [[differential form|differential one-form]] on ''M'' with
:<math> \|b\|_a := \sqrt{a^{ij}b_i b_j} < 1,</math>
where <math>(a^{ij})</math> is the [[inverse matrix]] of <math>(a_{ij})</math> and the [[Einstein notation]] is used. Then
:<math> F(x,v) := \sqrt{a_{ij}(x)v^iv^j} + b_i(x)v^i</math>
defines a '''Randers metric''' on ''M'' and (''M'',''F'') is a '''Randers manifold''', a special case of a non-reversible Finsler manifold.<ref>{{cite journal |first=G. |last=Randers |year=1941 |title=On an Asymmetrical Metric in the Four-Space of General Relativity |journal=[[Physical Review|Phys. Rev.]] |volume=59 |issue=2 |pages=195–199 |doi=10.1103/PhysRev.59.195 }}</ref>
 
<!--===Kropina manifolds===
'''F'''^3 = (''M'',''M''',''F'') is a Kropina manifold (after V. K. Kropina (1959)).-->
 
===Smooth quasimetric spaces===
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'',&nbsp;φ) of ''M'' and a constant ''C''&nbsp;≥&nbsp;1 such that for every ''x'',''y''&nbsp;∈&nbsp;''U''
:: <math> \frac{1}{C}\|\varphi(y)-\varphi(x)\| \leq d(x,y) \leq C\|\varphi(y)-\varphi(x)\|.</math>
* The function ''d''&nbsp;:&nbsp;''M''&nbsp;×&nbsp;''M''&nbsp;→[0,∞[ is [[smooth function|smooth]] in some punctured neighborhood of the diagonal.
 
Then one can define a Finsler function ''F''&nbsp;:&nbsp;''TM''&nbsp;→[0,∞[  by
 
:<math>F(x,v) := \lim_{t\to 0+} \frac{d(\gamma(0),\gamma(t))}{t},</math>
 
where ''&gamma;'' is any curve in ''M'' with ''&gamma;''(0)&nbsp;=&nbsp;''x'' and ''&gamma;'''(0)&nbsp;=&nbsp;v. The Finsler function ''F'' obtained in this way restricts to an asymmetric (typically non-Minkowski) norm on each tangent space of ''M''. The [[intrinsic metric|induced intrinsic metric]] {{nowrap|''d''<sub>''L''</sub>:&nbsp;''M''&nbsp;×&nbsp;''M''&nbsp;→&nbsp;[0,&nbsp;∞]}} of the original [[quasimetric]] can be recovered from
 
:<math> 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\},</math>
 
and in fact any Finsler function ''F''&nbsp;:&nbsp;''TM''&nbsp;→&nbsp;<nowiki>[</nowiki>0,&nbsp;∞<nowiki>)</nowiki> defines an [[intrinsic metric|intrinsic]] [[quasimetric]] ''d''<sub>''L''</sub> on ''M'' by this formula.
 
==Geodesics==
Due to the homogeneity of ''F'' the length
 
:<math>L[\gamma]:=\int_a^b F(\gamma(t),\dot{\gamma}(t))\, dt</math>
 
of a [[differentiable curve]] ''γ'':[''a'',''b'']→''M'' in ''M'' is invariant under positively oriented [[Parametrization|reparametrizations]]. A constant speed curve ''γ'' is a [[geodesic]] of a Finsler manifold if its short enough segments ''γ''|<sub>[''c'',''d'']</sub> are length-minimizing in ''M'' from ''γ''(''c'') to ''γ''(''d''). Equivalently, ''γ'' is a geodesic if it is stationary for the energy functional
 
:<math>E[\gamma]:=\frac{1}{2}\int_a^b F^2(\gamma(t),\dot{\gamma}(t))\, dt</math>
 
in the sense that its [[functional derivative]] vanishes among differentiable curves {{nowrap|''&gamma;'':[''a'',''b'']&rarr;''M''}} with fixed endpoints ''γ''(''a'')=''x'' and ''γ''(''b'')=''y''.
 
===Canonical spray structure on a Finsler manifold===
The [[Euler–Lagrange equation]] for the energy functional ''E''[''γ''] reads in the local coordinates (''x''<sup>1</sup>,...,''x''<sup>n</sup>,''v''<sup>1</sup>,...,''v''<sup>n</sup>) of ''TM'' as
 
:<math>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,
</math>
 
where ''k''=1,...,''n'' and ''g''<sub>ij</sub> is the coordinate representation of the fundamental tensor, defined as
 
:<math>
g_{ij}(x,v) := g_v\left(\tfrac{\partial}{\partial x^i}\big|_x,\tfrac{\partial}{\partial x^j}\big|_x\right).
</math>
 
Assuming the [[Convex function#Strongly convex functions|strong convexity]] of ''F''<sup>2</sup>(''x,v'') with respect to ''v''&isin;''T<sub>x</sub>M'', the matrix ''g''<sub>''ij''</sub>(''x'',''v'') is invertible and its inverse is denoted by ''g''<sup>''ij''</sup>(''x'',''v''). Then {{nobreak|''γ'':[''a'',''b'']&rarr;''M''}} is a geodesic of (''M'',''F'') if and only if its tangent curve {{nobreak|''γ''':[''a'',''b'']→''TM''&nbsp;\0}} is an [[integral curve]] of the [[vector field|smooth vector field]] ''H'' on ''TM''&nbsp;\0 locally defined by
 
:<math>
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)},
</math>
 
where the local spray coefficients ''G''<sup>i</sup> are given by
 
:<math>
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.
</math>
 
The vector field ''H'' on ''TM''/0 satisfies ''JH''&nbsp;=&nbsp;''V'' and [''V'',''H'']&nbsp;=&nbsp;''H'', where ''J'' and ''V'' are the [[Double tangent bundle#Canonical tensor fields on the tangent bundle|canonical endomorphism]] and the [[Double tangent bundle#Canonical tensor fields on the tangent bundle|canonical vector field]] on ''TM''&nbsp;\0. Hence, by definition, ''H'' is a [[Spray (mathematics)|spray]] on&nbsp;''M''. The spray ''H'' defines a [[Ehresmann connection|nonlinear connection]] on the [[fibre bundle]] {{nowrap|''TM''&nbsp;\0&nbsp;→&nbsp;''M''}} through the [[Ehresmann connection|vertical projection]]
 
:<math> v:T(TM\setminus 0)\to T(TM\setminus 0) \quad ; \quad v := \tfrac{1}{2}\big( I + \mathcal L_H J \big).</math>
 
In analogy with the [[Riemannian manifold|Riemannian]] case, there is a version
 
:<math>D_{\dot\gamma}D_{\dot\gamma}X(t) + R_{\dot\gamma}(\dot\gamma(t),X(t)) = 0</math>
 
of the [[Jacobi equation]] for a general spray structure (''M'',''H'') in terms of the [[Ehresmann connection|Ehresmann curvature]] and
[[Double tangent bundle#Nonlinear covarient derivatives on smooth manifolds|nonlinear covariant derivative]].
 
===Uniqueness and minimizing properties of geodesics===
By [[Hopf–Rinow theorem]] there always exist length minimizing curves (at least in small enough neighborhoods) on (''M'',&nbsp;''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 ''F''<sup>2</sup> there exists a unique maximal geodesic ''γ'' with ''γ''(0)&nbsp;=&nbsp;x and ''γ'''(0)&nbsp;=&nbsp;v for any (''x'',&nbsp;''v'')&nbsp;∈&nbsp;''TM''&nbsp;\&nbsp;0 by the uniqueness of [[integral curve]]s.
 
If ''F''<sup>2</sup> is strongly convex, geodesics ''&gamma;''&nbsp;:&nbsp;[0,&nbsp;''b'']&nbsp;→&nbsp;''M'' are length-minimizing among nearby curves until the first point ''&gamma;''(''s'') [[conjugate point|conjugate]] to ''&gamma;''(0) along ''&gamma;'', and for ''t''&nbsp;>&nbsp;''s'' there always exist shorter curves from ''&gamma;''(0) to ''&gamma;''(''t'') near ''&gamma;'', as in the [[Riemannian manifold|Riemannian]] case.
 
==Notes==
{{reflist}}
 
==References==
 
*{{Citation | editor1-last=Antonelli | editor1-first=P. L. | title=Handbook of Finsler geometry. Vol. 1, 2 | url=http://books.google.com/books?id=b2B5_IUvPJgC | publisher=Kluwer Academic Publishers | location=Boston | isbn=978-1-4020-1557-1 | mr=2067663 | year=2003}}
* D. Bao, [[S. S. Chern]] and Z. Shen, ''An Introduction to Riemann–Finsler Geometry,'' Springer-Verlag, 2000. ISBN 0-387-98948-X.
*{{Citation | last1=Cartan | first1=Elie | author1-link=Élie Cartan | title=Sur les espaces de Finsler | zbl=0006.22501 | year=1933 | journal=C. R. Acad. Sci., Paris  | volume=196 | pages=582–586}}
* [http://www.ams.org/notices/199609/chern.pdf S. Chern: ''Finsler geometry is just Riemannian geometry without the quadratic restriction'', Notices AMS, 43 (1996), pp. 959–63.]
*{{Citation | last1=Finsler | first1=Paul | title=Über Kurven und Flächen in allgemeinen Räumen | publisher=Göttingen | series=Dissertation | jfm=46.1131.02 | year=1918}} (Reprinted by Birkhäuser (1951))
* H. Rund. ''The Differential Geometry of Finsler Spaces,'' Springer-Verlag, 1959. ASIN B0006AWABG.
* Z. Shen, ''Lectures on Finsler Geometry,'' World Scientific Publishers, 2001. ISBN 981-02-4531-9.
 
==External links==
* {{springer|title=Finsler space, generalized|id=p/f040420}}
* Z. Shen's [http://www.math.iupui.edu/~zshen/Finsler/ Finsler Geometry Website].
* [http://finsler.blogspot.com/ The (New) Finsler Newsletter]
 
[[Category:Finsler geometry]]
[[Category:Smooth manifolds]]

Latest revision as of 16:13, 18 July 2014

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