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Cotangent bundle

From Wikipedia, the free encyclopedia
Vector bundle of cotangent spaces at every point in a manifold

Inmathematics, especiallydifferential geometry, thecotangent bundle of asmooth manifold is thevector bundle of all thecotangent spaces at every point in the manifold. It may be described also as thedual bundle to thetangent bundle. This may be generalized tocategories with more structure than smooth manifolds, such ascomplex manifolds, or (in the form of cotangent sheaf)algebraic varieties orschemes. In the smooth case, any Riemannian metric or symplectic form gives an isomorphism between the cotangent bundle and the tangent bundle, but they are not in general isomorphic in other categories.

Formal definition viadiagonal morphism

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There are several equivalent ways to define the cotangent bundle.One way is through adiagonal mappingΔ{\displaystyle \Delta } andgerms.

LetM{\displaystyle M} be asmooth manifold and letM×M{\displaystyle M\times M} be theCartesian product ofM{\displaystyle M} with itself. Thediagonal mappingΔ{\displaystyle \Delta } sends a pointp{\displaystyle p} inM{\displaystyle M} to the point(p,p){\displaystyle (p,p)} ofM×M{\displaystyle M\times M}. The image ofΔ{\displaystyle \Delta } is called the diagonal. LetI{\displaystyle {\mathcal {I}}} be thesheaf ofgerms of smooth functions onM×M{\displaystyle M\times M} which vanish on the diagonal. Then thequotient sheafI/I2{\displaystyle {\mathcal {I}}/{\mathcal {I}}^{2}} consists of equivalence classes of functions which vanish on the diagonal modulo higher order terms. Thecotangent sheaf is defined as thepullback of this sheaf toM{\displaystyle M}:

ΓTM=Δ(I/I2).{\displaystyle \Gamma T^{*}M=\Delta ^{*}\left({\mathcal {I}}/{\mathcal {I}}^{2}\right).}

ByTaylor's theorem, this is alocally free sheaf of modules with respect to the sheaf of germs of smooth functions ofM{\displaystyle M}. Thus it defines avector bundle onM{\displaystyle M}: thecotangent bundle.

Smoothsections of the cotangent bundle are called (differential)one-forms.

Contravariance properties

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A smooth morphismϕ:MN{\displaystyle \phi \colon M\to N} of manifolds induces apullback sheafϕTN{\displaystyle \phi ^{*}T^{*}N} onM. There is aninduced map of vector bundlesϕ(TN)TM{\displaystyle \phi ^{*}(T^{*}N)\to T^{*}M}.

Examples

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The tangent bundle of the vector spaceRn{\displaystyle \mathbb {R} ^{n}} isTRn=Rn×Rn{\displaystyle T\,\mathbb {R} ^{n}=\mathbb {R} ^{n}\times \mathbb {R} ^{n}}, and the cotangent bundle isTRn=Rn×(Rn){\displaystyle T^{*}\mathbb {R} ^{n}=\mathbb {R} ^{n}\times (\mathbb {R} ^{n})^{*}}, where(Rn){\displaystyle (\mathbb {R} ^{n})^{*}} denotes thedual space of covectors, linear functionsv:RnR{\displaystyle v^{*}:\mathbb {R} ^{n}\to \mathbb {R} }.

Given a smooth manifoldMRn{\displaystyle M\subset \mathbb {R} ^{n}} embedded as ahypersurface represented by the vanishing locus of a functionfC(Rn),{\displaystyle f\in C^{\infty }(\mathbb {R} ^{n}),} with the condition thatf0,{\displaystyle \nabla f\neq 0,} the tangent bundle is

TM={(x,v)TRn : f(x)=0, dfx(v)=0},{\displaystyle TM=\{(x,v)\in T\,\mathbb {R} ^{n}\ :\ f(x)=0,\ \,df_{x}(v)=0\},}

wheredfxTxM{\displaystyle df_{x}\in T_{x}^{*}M} is thedirectional derivativedfx(v)=f(x)v{\displaystyle df_{x}(v)=\nabla \!f(x)\cdot v}. By definition, the cotangent bundle in this case is

TM={(x,v)TRn : f(x)=0, vTxM},{\displaystyle T^{*}M={\bigl \{}(x,v^{*})\in T^{*}\mathbb {R} ^{n}\ :\ f(x)=0,\ v^{*}\in T_{x}^{*}M{\bigr \}},}

whereTxM={vTxRn : dfx(v)=0}.{\displaystyle T_{x}^{*}M=\{v\in T_{x}\mathbb {R} ^{n}\ :\ df_{x}(v)=0\}^{*}.} Since every covectorvTxM{\displaystyle v^{*}\in T_{x}^{*}M} corresponds to a unique vectorvTxM{\displaystyle v\in T_{x}M} for whichv(u)=vu,{\displaystyle v^{*}(u)=v\cdot u,} for an arbitraryuTxM,{\displaystyle u\in T_{x}M,}

TM={(x,v)TRn : f(x)=0, vTxRn, dfx(v)=0}.{\displaystyle T^{*}M={\bigl \{}(x,v^{*})\in T^{*}\mathbb {R} ^{n}\ :\ f(x)=0,\ v\in T_{x}\mathbb {R} ^{n},\ df_{x}(v)=0{\bigr \}}.}

The cotangent bundle as phase space

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Since the cotangent bundleX=TM{\displaystyle X=T^{*}M} is avector bundle, it can be regarded as a manifold in its own right. Because at each point the tangent directions ofM{\displaystyle M} can be paired with their dual covectors in the fiber,X{\displaystyle X} possesses a canonical one-formθ{\displaystyle \theta } called thetautological one-form, discussed below. Theexterior derivative ofθ{\displaystyle \theta } is asymplectic 2-form, out of which a non-degeneratevolume form can be built forX{\displaystyle X}. For example, as a resultX{\displaystyle X} is always anorientable manifold (the tangent bundleTX{\displaystyle TX} is an orientable vector bundle). A special set ofcoordinates can be defined on the cotangent bundle; these are called thecanonical coordinates. Because cotangent bundles can be thought of assymplectic manifolds, any real function on the cotangent bundle can be interpreted to be aHamiltonian; thus the cotangent bundle can be understood to be aphase space on whichHamiltonian mechanics plays out.

The tautological one-form

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Main article:Tautological one-form

The cotangent bundle carries a canonical one-form θ also known as thesymplectic potential,Poincaré1-form, orLiouville1-form. This means that if we regardT*M as a manifold in its own right, there is a canonicalsection of the vector bundleT*(T*M) overT*M.

This section can be constructed in several ways. The most elementary method uses local coordinates. Suppose thatxi are local coordinates on the base manifoldM. In terms of these base coordinates, there are fibre coordinatespi : a one-form at a particular point ofT*M has the formpi dxi (Einstein summation convention implied). So the manifoldT*M itself carries local coordinates (xi,pi) where thex's are coordinates on the base and thep's are coordinates in the fibre. The canonical one-form is given in these coordinates by

θ(x,p)=i=1npidxi.{\displaystyle \theta _{(x,p)}=\sum _{i=1}^{n}p_{i}\,dx^{i}.}

Intrinsically, the value of the canonical one-form in each fixed point ofT*M is given as apullback. Specifically, suppose thatπ :T*MM is theprojection of the bundle. Taking a point inTx*M is the same as choosing of a pointx inM and a one-form ω atx, and the tautological one-form θ assigns to the point (x, ω) the value

θ(x,ω)=πω.{\displaystyle \theta _{(x,\omega )}=\pi ^{*}\omega .}

That is, for a vectorv in the tangent bundle of the cotangent bundle, the application of the tautological one-form θ tov at (x, ω) is computed by projectingv into the tangent bundle atx usingdπ :T(T*M) →TM and applying ω to this projection. Note that the tautological one-form is not a pullback of a one-form on the baseM.

Symplectic form

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The cotangent bundle has a canonicalsymplectic 2-form on it, as anexterior derivative of thetautological one-form, thesymplectic potential. Proving that this form is, indeed, symplectic can be done by noting that being symplectic is a local property: since the cotangent bundle is locally trivial, this definition need only be checked onRn×Rn{\displaystyle \mathbb {R} ^{n}\times \mathbb {R} ^{n}}. But there the one form defined is the sum ofyidxi{\displaystyle y_{i}\,dx_{i}}, and the differential is the canonical symplectic form, the sum ofdyidxi{\displaystyle dy_{i}\land dx_{i}}.

Phase space

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If the manifoldM{\displaystyle M} represents the set of possible positions in adynamical system, then the cotangent bundleTM{\displaystyle \!\,T^{*}\!M} can be thought of as the set of possiblepositions andmomenta. For example, this is a way to describe thephase space of a pendulum. The state of the pendulum is determined by its position (an angle) and its momentum (or equivalently, its velocity, since its mass is constant). The entire state space looks like a cylinder, which is the cotangent bundle of the circle. The above symplectic construction, along with an appropriateenergy function, gives a complete determination of the physics of system. SeeHamiltonian mechanics and the article ongeodesic flow for an explicit construction of the Hamiltonian equations of motion.

See also

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References

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Basic concepts
Main theorems(list)
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