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Symplectic manifold

From Wikipedia, the free encyclopedia
Type of manifold in differential geometry

Indifferential geometry, a subject ofmathematics, asymplectic manifold is asmooth manifold,M{\displaystyle M}, equipped with aclosednondegeneratedifferential 2-formω{\displaystyle \omega }, called the symplectic form. The study of symplectic manifolds is calledsymplectic geometry or symplectic topology. Symplectic manifolds arise naturally in abstract formulations ofclassical mechanics andanalytical mechanics as thecotangent bundles of manifolds. For example, in theHamiltonian formulation of classical mechanics, which provides one of the major motivations for the field, the set of all possible configurations of a system is modeled as a manifold, and this manifold's cotangent bundle describes thephase space of the system.

Motivation

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Symplectic manifolds arise fromclassical mechanics; in particular, they are a generalization of thephase space of a closed system.[1] In the same way theHamilton equations allow one to derive the time evolution of a system from a set ofdifferential equations, the symplectic form should allow one to obtain avector field describing the flow of the system from the differentialdH{\displaystyle dH} of a Hamiltonian functionH{\displaystyle H}.[2] So we require a linear mapTMTM{\displaystyle TM\rightarrow T^{*}M} from thetangent manifoldTM{\displaystyle TM} to thecotangent manifoldTM{\displaystyle T^{*}M}, or equivalently, an element ofTMTM{\displaystyle T^{*}M\otimes T^{*}M}. Lettingω{\displaystyle \omega } denote asection ofTMTM{\displaystyle T^{*}M\otimes T^{*}M}, the requirement thatω{\displaystyle \omega } benon-degenerate ensures that for every differentialdH{\displaystyle dH} there is a unique corresponding vector fieldVH{\displaystyle V_{H}} such thatdH=ω(VH,){\displaystyle dH=\omega (V_{H},\cdot )}. Since one desires the Hamiltonian to be constant along flow lines, one should haveω(VH,VH)=dH(VH)=0{\displaystyle \omega (V_{H},V_{H})=dH(V_{H})=0}, which implies thatω{\displaystyle \omega } isalternating and hence a 2-form. Finally, one makes the requirement thatω{\displaystyle \omega } should not change under flow lines, i.e. that theLie derivative ofω{\displaystyle \omega } alongVH{\displaystyle V_{H}} vanishes. ApplyingCartan's formula, this amounts to (hereιX{\displaystyle \iota _{X}} is theinterior product):

LVH(ω)=0d(ιVHω)+ιVHdω=d(dH)+dω(VH)=dω(VH)=0{\displaystyle {\mathcal {L}}_{V_{H}}(\omega )=0\;\Leftrightarrow \;\mathrm {d} (\iota _{V_{H}}\omega )+\iota _{V_{H}}\mathrm {d} \omega =\mathrm {d} (\mathrm {d} \,H)+\mathrm {d} \omega (V_{H})=\mathrm {d} \omega (V_{H})=0}

so that, on repeating this argument for different smooth functionsH{\displaystyle H} such that the correspondingVH{\displaystyle V_{H}} span the tangent space at each point the argument is applied at, we see that the requirement for the vanishing Lie derivative along flows ofVH{\displaystyle V_{H}} corresponding to arbitrary smoothH{\displaystyle H} is equivalent to the requirement thatω should beclosed.

Definition

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LetM{\displaystyle M} be a smoothmanifold. Asymplectic form onM{\displaystyle M} is a closed non-degenerate differential2-formω{\displaystyle \omega }.[3][4] Here, non-degenerate means that for every pointpM{\displaystyle p\in M}, the skew-symmetric pairing on thetangent spaceTpM{\displaystyle T_{p}M} defined byω{\displaystyle \omega } is non-degenerate. That is to say, if there exists anXTpM{\displaystyle X\in T_{p}M} such thatω(X,Y)=0{\displaystyle \omega (X,Y)=0} for allYTpM{\displaystyle Y\in T_{p}M}, thenX=0{\displaystyle X=0}. The closed condition means that theexterior derivative ofω{\displaystyle \omega } vanishes.[3][4]

Asymplectic manifold is a pair(M,ω){\displaystyle (M,\omega )} whereM{\displaystyle M} is a smooth manifold andω{\displaystyle \omega } is a symplectic form. Assigning a symplectic form toM{\displaystyle M} is referred to as givingM{\displaystyle M} asymplectic structure. Since in odd dimensions,skew-symmetric matrices are always singular, nondegeneracy implies thatdimM{\displaystyle \dim M} is even.

By nondegeneracy,ω{\displaystyle \omega } can be used to define a pair ofmusical isomorphismsω:TMTM,ω:TMTM{\displaystyle \omega ^{\flat }:TM\rightarrow T^{*}M,\omega ^{\sharp }:T^{*}M\rightarrow TM}, such thatω(X,Y)=ω(X)(Y){\displaystyle \omega (X,Y)=\omega ^{\flat }(X)(Y)} for any two vector fieldsX,Y{\displaystyle X,Y}, andωω=Id{\displaystyle \omega ^{\sharp }\circ \omega ^{\flat }=\operatorname {Id} }.

A symplectic manifold(M,ω){\displaystyle (M,\omega )} isexact iff the symplectic formω{\displaystyle \omega } isexact, i.e. equal toω=dθ{\displaystyle \omega =-d\theta } for some 1-formθ{\displaystyle \theta }. The area 2-form on the 2-sphere is an inexact symplectic form, by thehairy ball theorem.

ByDarboux's theorem, around any pointp{\displaystyle p} there exists a local coordinate system, in whichω=Σidpidqi{\displaystyle \omega =\Sigma _{i}dp_{i}\wedge dq^{i}}, where d denotes theexterior derivative and ∧ denotes theexterior product. This form is called thePoincaré two-form or thecanonical two-form. Thus, we can locally think ofM as being thecotangent bundleTRn{\displaystyle T^{*}\mathbb {R} ^{n}} and generated by the correspondingtautological 1-formθ=Σipidqi,ω=dθ{\displaystyle \theta =\Sigma _{i}p_{i}dq^{i},\;\omega =d\theta }.

A (local)Liouville form is any (locally defined)λ{\displaystyle \lambda } such thatω=dλ{\displaystyle \omega =d\lambda }. A vector fieldX{\displaystyle X} is (locally)Liouville iffLXω=ω{\displaystyle {\mathcal {L}}_{X}\omega =\omega }. ByCartan's magic formula, this is equivalent tod(ω(X,))=ω{\displaystyle d(\omega (X,\cdot ))=\omega }. A Liouville vector field can thus be interpreted as a way to recover a (local) Liouville form. By Darboux's theorem, around any point there exists a local Liouville form, though it might not exist globally.

Given any smooth functionf:MR{\displaystyle f:M\to \mathbb {R} }, itsHamiltonian vector field is the unique vector fieldXf{\displaystyle X_{f}} satisfyingω(Xf,)=df{\displaystyle \omega (X_{f},\cdot )=df}. The set of all Hamiltonian vector fields make up aLie algebra, and is written as(Ham(M),[,]){\displaystyle (\operatorname {Ham} (M),[\cdot ,\cdot ])} where[,]{\displaystyle [\cdot ,\cdot ]} is theLie bracket.

Given any two smooth functionsf,g:MR{\displaystyle f,g:M\to \mathbb {R} }, theirPoisson bracket is defined by{f,g}=ω(Xg,Xf){\displaystyle \{f,g\}=\omega (X_{g},X_{f})}. This makes any symplectic manifold into aPoisson manifold. ThePoisson bivector is abivector fieldπ{\displaystyle \pi } defined by{f,g}=π(dfdg){\displaystyle \{f,g\}=\pi (df\wedge dg)}, or equivalently, byπ:=ω1{\displaystyle \pi :=\omega ^{-1}}. The Poisson bracket and Lie bracket are related byX{f,g}=[Xf,Xg]{\textstyle X_{\{f,g\}}=[X_{f},X_{g}]}.

Submanifolds

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There are several natural geometric notions ofsubmanifold of a symplectic manifold(M,ω){\displaystyle (M,\omega )}. LetNM{\displaystyle N\subset M} be a submanifold. It is

The conditions can also be defined bydifferential algebra using Poisson brackets. LetIN:={f:MR:f|N=0}{\displaystyle I_{N}:=\{f:M\to \mathbb {R} :f|_{N}=0\}} be thedifferential ideal of functions vanishing onN{\displaystyle N}, thenN{\displaystyle N} is isotropic iff{IN,IN}IN{\displaystyle \{I_{N},I_{N}\}\subset I_{N}}, coisotropic iff{IN,C(M)}IN{\displaystyle \{I_{N},C^{\infty }(M)\}\subset I_{N}}, Lagrangian iff the induced Poisson bracket on the quotient algebraC(M)/IN{\displaystyle C^{\infty }(M)/I_{N}} is zero, and symplectic iff the induced Poisson bracket on the quotient algebraC(M)/IN{\displaystyle C^{\infty }(M)/I_{N}} is nondegenerate.

Lagrangian submanifolds

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Lagrangian submanifolds are the most important submanifolds.Weinstein proposed the "symplectic creed":Everything is a Lagrangian submanifold. By that, he means that everything in symplectic geometry is most naturally expressed in terms of Lagrangian submanifolds.[5]

ALagrangian fibration of a symplectic manifoldM is afibration where all of thefibers are Lagrangian submanifolds.

Given a submanifoldNM{\displaystyle N\subset M} of codimension 1, thecharacteristic line distribution on it is the duals to its tangent spaces:TpNω{\displaystyle T_{p}N^{\omega }}. If there also exists a Liouville vector fieldX{\displaystyle X} in a neighborhood of it that istransverse to it. In this case, letα:=ω(X,)|N{\displaystyle \alpha :=\omega (X,\cdot )|_{N}}, then(N,α){\displaystyle (N,\alpha )} is acontact manifold, and we say it is acontact type submanifold. In this case, theReeb vector field is tangent to the characteristic line distribution.

Ann-submanifold is locally specified by a smooth functionu:RnM{\displaystyle u:\mathbb {R} ^{n}\to M}. It is a Lagrangian submanifold ifω(i,j)=0{\displaystyle \omega (\partial _{i},\partial _{j})=0} for alli,j1:n{\displaystyle i,j\in 1:n}. If locally there is a canonical coordinate system(q,p){\displaystyle (q,p)}, then the condition is equivalent to[u,v]p,q=i=1n(qiupivpiuqiv)=0,i,j1:n{\displaystyle [u,v]_{p,q}=\sum _{i=1}^{n}\left({\frac {\partial q_{i}}{\partial u}}{\frac {\partial p_{i}}{\partial v}}-{\frac {\partial p_{i}}{\partial u}}{\frac {\partial q_{i}}{\partial v}}\right)=0,\quad \forall i,j\in 1:n}where[,]p,q{\displaystyle [\cdot ,\cdot ]_{p,q}} is theLagrange bracket in this coordinate system.

Given any differentiable functionf:MR{\displaystyle f:M\to \mathbb {R} }, its differentialdf{\displaystyle df} has a graph inTM{\displaystyle T^{*}M}. The graph is a Lagrangian submanifold. Conversely, if a Lagrangian submanifoldLTM{\displaystyle L\subset T^{*}M} projects down toM{\displaystyle M} diffeomorphically (i.e. the projection mapπ:TMM{\displaystyle \pi :T^{*}M\to M}, when restricted to the submanifold, is a diffeomorphism), then it is the graph of somedf{\displaystyle df} for somef:MR{\displaystyle f:M\to \mathbb {R} }. In such a case,f{\displaystyle f} is thegenerating function of a Lagrangian manifold.

This example shows that Lagrangian submanifolds satisfy anh-principle, exist in great abundance, and are not rigid. The classification of symplectic manifolds is done viaFloer homology—this is an application ofMorse theory to theaction functional for maps between Lagrangian submanifolds. In physics, the action describes the time evolution of a physical system; here, it can be taken as the description of the dynamics of branes.

Lagrangian mapping

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See also:symplectic category

LetL be a Lagrangian submanifold of a symplectic manifold (K,ω) given by animmersioni :LK (i is called aLagrangian immersion). Letπ :KB give a Lagrangian fibration ofK. The composite(πi) :LKB is aLagrangian mapping. Thecritical value set ofπi is called acaustic.

Two Lagrangian maps(π1i1) :L1K1B1 and(π2i2) :L2K2B2 are calledLagrangian equivalent if there existdiffeomorphismsσ,τ andν such that both sides of the diagram given on the rightcommute, andτ preserves the symplectic form.[4] Symbolically:

τi1=i2σ, νπ1=π2τ, τω2=ω1,{\displaystyle \tau \circ i_{1}=i_{2}\circ \sigma ,\ \nu \circ \pi _{1}=\pi _{2}\circ \tau ,\ \tau ^{*}\omega _{2}=\omega _{1}\,,}

whereτω2 denotes thepull back ofω2 byτ.

Symmetries

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Main article:Symplectomorphism

A mapf:(M,ω)(M,ω){\displaystyle f:(M,\omega )\to (M',\omega ')} between symplectic manifolds is asymplectomorphism when it preserves the symplectic structure, i.e. thepullback is the samefω=ω{\displaystyle f^{*}\omega '=\omega }. The most important symplectomorphisms are symplectic flows, i.e. ones generated by integrating a vector field on(M,ω){\displaystyle (M,\omega )}.

Given a vector fieldX{\displaystyle X} on(M,ω){\displaystyle (M,\omega )}, it generates a symplectic flow iffLXω=0{\displaystyle {\mathcal {L}}_{X}\omega =0}. Such vector fields are calledsymplectic. Any Hamiltonian vector field is symplectic, and conversely, any symplectic vector field islocally Hamiltonian.

A property that is preserved under all symplectomorphisms is asymplectic invariant. In the spirit ofErlangen program, symplectic geometry is the study of symplectic invariants.

Examples

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The standard symplectic structure

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Main article:Symplectic vector space

Let{v1,,v2n}{\displaystyle \{v_{1},\ldots ,v_{2n}\}} be a basis forR2n.{\displaystyle \mathbb {R} ^{2n}.} We define our symplectic formω{\displaystyle \omega } on this basis as follows:

ω(vi,vj)={1ji=n with 1in1ij=n with 1jn0otherwise{\displaystyle \omega (v_{i},v_{j})={\begin{cases}1&j-i=n{\text{ with }}1\leqslant i\leqslant n\\-1&i-j=n{\text{ with }}1\leqslant j\leqslant n\\0&{\text{otherwise}}\end{cases}}}

In this case the symplectic form reduces to a simplequadratic form. IfIn{\displaystyle I_{n}} denotes then×n{\displaystyle n\times n}identity matrix then the matrix,Ω{\displaystyle \Omega }, of this quadratic form is given by the2n×2n{\displaystyle 2n\times 2n}block matrix:

Ω=(0InIn0).{\displaystyle \Omega ={\begin{pmatrix}0&I_{n}\\-I_{n}&0\end{pmatrix}}.}

That is,

ω=dx1dy1++dxndyn.{\displaystyle \omega =\mathrm {d} x_{1}\wedge \mathrm {d} y_{1}+\dotsb +\mathrm {d} x_{n}\wedge \mathrm {d} y_{n}.}

It has a fibration by Lagrangian submanifolds with fixed value ofy{\displaystyle y}, i.e.{Rn×{y}:yRn}{\displaystyle \{\mathbb {R} ^{n}\times \{y\}:y\in \mathbb {R} ^{n}\}}.

A Liouville form for this isλ=12i(xidyiyidxi){\textstyle \lambda ={\frac {1}{2}}\sum _{i}\left(x_{i}dy_{i}-y_{i}dx_{i}\right)} andω=dλ{\textstyle \omega =d\lambda }, the Liouville vector field isY=12i(xixi+yiyi),{\displaystyle Y={\frac {1}{2}}\sum _{i}\left(x_{i}\partial _{x_{i}}+y_{i}\partial _{y_{i}}\right),}the radial field. Another Liouville form isΣixidyi{\displaystyle \Sigma _{i}x_{i}dy_{i}}, with Liouville vector fieldY=ixixi{\textstyle Y=\sum _{i}x_{i}\partial _{x_{i}}}.

Cotangent bundles

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LetQ{\displaystyle Q} be a smooth manifold of dimensionn{\displaystyle n}. Then the total space of thecotangent bundleTQ{\displaystyle T^{*}Q} has a natural symplectic form, called the Poincaré two-form or thecanonical symplectic form

ω=i=1ndpidqi{\displaystyle \omega =\sum _{i=1}^{n}dp_{i}\wedge dq^{i}}

Here(q1,,qn){\displaystyle (q^{1},\ldots ,q^{n})} are any local coordinates onQ{\displaystyle Q} and(p1,,pn){\displaystyle (p_{1},\ldots ,p_{n})} are fibrewise coordinates with respect to the cotangent vectorsdq1,,dqn{\displaystyle dq^{1},\ldots ,dq^{n}}. Cotangent bundles are the naturalphase spaces of classical mechanics. The point of distinguishing upper and lower indexes is driven by the case of the manifold having ametric tensor, as is the case forRiemannian manifolds. Upper and lower indexes transform contra and covariantly under a change of coordinate frames. The phrase "fibrewise coordinates with respect to the cotangent vectors" is meant to convey that the momentapi{\displaystyle p_{i}} are "soldered" to the velocitiesdqi{\displaystyle dq^{i}}. The soldering is an expression of the idea that velocity and momentum are colinear, in that both move in the same direction, and differ by a scale factor.

The tautological 1-formλ=ipidqi{\displaystyle \lambda =\sum _{i}p_{i}dq^{i}} has Liouville vector fieldY=ipipi{\displaystyle Y=\sum _{i}p_{i}\partial _{p_{i}}}, the fiberwise radial field. Its flow dilates covectors:(q,p)(q,etp){\textstyle (q,p)\mapsto \left(q,e^{t}p\right)}.

The zero section of the cotangent bundle is Lagrangian. For example, let

X={(x,y)R2:y2x=0}.{\displaystyle X=\{(x,y)\in \mathbb {R} ^{2}:y^{2}-x=0\}.}

Then, we can presentTX{\displaystyle T^{*}X} as

TX={(x,y,dx,dy)R4:y2x=0,2ydydx=0}{\displaystyle T^{*}X=\{(x,y,\mathrm {d} x,\mathrm {d} y)\in \mathbb {R} ^{4}:y^{2}-x=0,2y\mathrm {d} y-\mathrm {d} x=0\}}

where we are treating the symbolsdx,dy{\displaystyle \mathrm {d} x,\mathrm {d} y} as coordinates ofR4=TR2{\displaystyle \mathbb {R} ^{4}=T^{*}\mathbb {R} ^{2}}. We can consider the subset where the coordinatesdx=0{\displaystyle \mathrm {d} x=0} anddy=0{\displaystyle \mathrm {d} y=0}, giving us the zero section. This example can be repeated for any manifold defined by the vanishing locus of smooth functionsf1,,fk{\displaystyle f_{1},\dotsc ,f_{k}} and their differentialsdf1,,dfk{\displaystyle \mathrm {d} f_{1},\dotsc ,df_{k}}.

Kähler manifolds

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AKähler manifold is a symplectic manifold equipped with a compatible integrable complex structure. They form a particular class ofcomplex manifolds. A large class of examples come from complexalgebraic geometry. Any smooth complexprojective varietyVCPn{\displaystyle V\subset \mathbb {CP} ^{n}} has a symplectic form which is the restriction of theFubini—Study form on theprojective spaceCPn{\displaystyle \mathbb {CP} ^{n}}.

A symplectic manifold endowed with ametric that iscompatible with the symplectic form is analmost Kähler manifold in the sense that the tangent bundle has analmost complex structure, but this need not beintegrable.

Almost-complex manifolds

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Riemannian manifolds with anω{\displaystyle \omega }-compatiblealmost complex structure are termedalmost-complex manifolds. They generalize Kähler manifolds, in that they need not beintegrable. That is, they do not necessarily arise from a complex structure on the manifold.

Special Lagrangian submanifolds

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The graph of asymplectomorphism in the product symplectic manifold(M ×M,ω × −ω) is Lagrangian. Their intersections display rigidity properties not possessed by smooth manifolds; theArnold conjecture gives the sum of the submanifold'sBetti numbers as a lower bound for the number of self intersections of a smooth Lagrangian submanifold, rather than theEuler characteristic in the smooth case.

In the case ofKähler manifolds (orCalabi–Yau manifolds) we can make a choiceΩ=Ω1+iΩ2{\displaystyle \Omega =\Omega _{1}+\mathrm {i} \Omega _{2}} onM{\displaystyle M} as a holomorphic n-form, whereΩ1{\displaystyle \Omega _{1}} is the real part andΩ2{\displaystyle \Omega _{2}} imaginary. A Lagrangian submanifoldL{\displaystyle L} is calledspecial if in addition to the above Lagrangian condition the restrictionΩ2{\displaystyle \Omega _{2}} toL{\displaystyle L} is vanishing. In other words, the real partΩ1{\displaystyle \Omega _{1}} restricted onL{\displaystyle L} leads the volume form onL{\displaystyle L}. The following examples are known as special Lagrangian submanifolds,

  1. complex Lagrangian submanifolds ofhyperkähler manifolds,
  2. fixed points of a real structure of Calabi–Yau manifolds.

InMorse theory, given aMorse functionf:MR{\displaystyle f:M\to \mathbb {R} } and for a small enoughε{\displaystyle \varepsilon } one can construct a Lagrangian submanifold given by the vanishing locusV(εdf)TM{\displaystyle \mathbb {V} (\varepsilon \cdot \mathrm {d} f)\subset T^{*}M}. For a generic Morse function we have a Lagrangian intersection given byMV(εdf)=Crit(f){\displaystyle M\cap \mathbb {V} (\varepsilon \cdot \mathrm {d} f)={\text{Crit}}(f)}.

TheSYZ conjecture deals with the study of special Lagrangian submanifolds inmirror symmetry; see (Hitchin 1999).

TheThomas–Yau conjecture predicts that the existence of a special Lagrangian submanifolds on Calabi–Yau manifolds in Hamiltonian isotopy classes of Lagrangians is equivalent to stability with respect to astability condition on theFukaya category of the manifold.

Generalizations

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  • Presymplectic manifolds generalize the symplectic manifolds by only requiringω{\displaystyle \omega } to be closed, but possibly degenerate. Any submanifold of a symplectic manifold inherits a presymplectic structure.
  • Poisson manifolds generalize the symplectic manifolds by preserving only thedifferential-algebraic structures of a symplectic manifold.
  • Dirac manifolds generalize Poisson manifolds and presymplectic manifolds by preserving even less structure. The definition is designed so that any submanifold of a Poisson manifold induces a Dirac manifold. They can be called "pre-Poisson" manifolds.
  • Amultisymplectic manifold of degreek is a manifold equipped with a closed nondegeneratek-form.[6]
  • Apolysymplectic manifold is a Legendre bundle provided with a polysymplectic tangent-valued(n+2){\displaystyle (n+2)}-form; it is utilized inHamiltonian field theory.[7]

See also

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Citations

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  1. ^Webster, Ben (9 January 2012)."What is a symplectic manifold, really?".
  2. ^Cohn, Henry."Why symplectic geometry is the natural setting for classical mechanics".
  3. ^abde Gosson, Maurice (2006).Symplectic Geometry and Quantum Mechanics. Basel: Birkhäuser Verlag. p. 10.ISBN 3-7643-7574-4.
  4. ^abcArnold, V. I.;Varchenko, A. N.;Gusein-Zade, S. M. (1985).The Classification of Critical Points, Caustics and Wave Fronts: Singularities of Differentiable Maps, Vol 1. Birkhäuser.ISBN 0-8176-3187-9.
  5. ^Weinstein, Alan (1981)."Symplectic geometry".Bulletin of the American Mathematical Society.5 (1):1–13.doi:10.1090/S0273-0979-1981-14911-9.ISSN 0273-0979.
  6. ^Cantrijn, F.; Ibort, L. A.; de León, M. (1999)."On the Geometry of Multisymplectic Manifolds".J. Austral. Math. Soc. Ser. A.66 (3):303–330.doi:10.1017/S1446788700036636.
  7. ^Giachetta, G.; Mangiarotti, L.;Sardanashvily, G. (1999). "Covariant Hamiltonian equations for field theory".Journal of Physics.A32 (38):6629–6642.arXiv:hep-th/9904062.Bibcode:1999JPhA...32.6629G.doi:10.1088/0305-4470/32/38/302.S2CID 204899025.

General and cited references

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Further reading

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Basic concepts
Main theorems(list)
Maps
Types of
manifolds
Tensors
Vectors
Covectors
Bundles
Connections
Related
Generalizations
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