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Tangent bundle


Informally, the tangent bundle of a manifold (which in this case is a circle) is obtained by considering all the tangent spaces (top), and joining them together in a smooth and non-overlapping manner (bottom).

A tangent bundle is the collection of all of the tangent spaces for all points on a manifold, structured in a way that it forms a new manifold itself. Formally, in differential geometry, the tangent bundle of a differentiable manifold

    M
  

{\displaystyle M}

is a manifold

    T
    M
  

{\displaystyle TM}

which assembles all the tangent vectors in

    M
  

{\displaystyle M}

. As a set, it is given by the disjoint union of the tangent spaces of

    M
  

{\displaystyle M}

. That is,

T M

            =
            
              ⨆
              
                x
                ∈
                M
              
            
            
              T
              
                x
              
            
            M
          
        
        
          
          
            
            =
            
              ⋃
              
                x
                ∈
                M
              
            
            
              {
              x
              }
            
            ×
            
              T
              
                x
              
            
            M
          
        
        
          
          
            
            =
            
              ⋃
              
                x
                ∈
                M
              
            
            
              {
              
                (
                x
                ,
                y
                )
                ∣
                y
                ∈
                
                  T
                  
                    x
                  
                
                M
              
              }
            
          
        
        
          
          
            
            =
            
              {
              
                (
                x
                ,
                y
                )
                ∣
                x
                ∈
                M
                ,
                
                y
                ∈
                
                  T
                  
                    x
                  
                
                M
              
              }
            
          
        
      
    
  

{\displaystyle {\begin{aligned}TM&=\bigsqcup _{x\in M}T_{x}M\\&=\bigcup _{x\in M}\left\{x\right\}\times T_{x}M\\&=\bigcup _{x\in M}\left\{(x,y)\mid y\in T_{x}M\right\}\\&=\left\{(x,y)\mid x\in M,\,y\in T_{x}M\right\}\end{aligned}}}

where

      T
      
        x
      
    
    M
  

{\displaystyle T_{x}M}

denotes the tangent space to

    M
  

{\displaystyle M}

at the point

    x
  

{\displaystyle x}

. So, an element of

    T
    M
  

{\displaystyle TM}

can be thought of as a pair

    (
    x
    ,
    v
    )
  

{\displaystyle (x,v)}

, where

    x
  

{\displaystyle x}

is a point in

    M
  

{\displaystyle M}

and

    v
  

{\displaystyle v}

is a tangent vector to

    M
  

{\displaystyle M}

at

    x
  

{\displaystyle x}

.

There is a natural projection

π : T M ↠ M

{\displaystyle \pi :TM\twoheadrightarrow M}

defined by

    π
    (
    x
    ,
    v
    )
    =
    x
  

{\displaystyle \pi (x,v)=x}

. This projection maps each element of the tangent space

      T
      
        x
      
    
    M
  

{\displaystyle T_{x}M}

to the single point

    x
  

{\displaystyle x}

.

The tangent bundle comes equipped with a natural topology (described in a section below). With this topology, the tangent bundle to a manifold is the prototypical example of a vector bundle (which is a fiber bundle whose fibers are vector spaces). A section of

    T
    M
  

{\displaystyle TM}

is a vector field on

    M
  

{\displaystyle M}

, and the dual bundle to

    T
    M
  

{\displaystyle TM}

is the cotangent bundle, which is the disjoint union of the cotangent spaces of

    M
  

{\displaystyle M}

. By definition, a manifold

    M
  

{\displaystyle M}

is parallelizable if and only if the tangent bundle is trivial. By definition, a manifold

    M
  

{\displaystyle M}

is framed if and only if the tangent bundle

    T
    M
  

{\displaystyle TM}

is stably trivial, meaning that for some trivial bundle

    E
  

{\displaystyle E}

the Whitney sum

    T
    M
    ⊕
    E
  

{\displaystyle TM\oplus E}

is trivial. For example, the n-dimensional sphere Sn is framed for all n, but parallelizable only for n = 1, 3, 7 (by results of Bott-Milnor and Kervaire).

One of the main roles of the tangent bundle is to provide a domain and range for the derivative of a smooth function. Namely, if

    f
    :
    M
    →
    N
  

{\displaystyle f:M\rightarrow N}

is a smooth function, with

    M
  

{\displaystyle M}

and

    N
  

{\displaystyle N}

smooth manifolds, its derivative is a smooth function

    D
    f
    :
    T
    M
    →
    T
    N
  

{\displaystyle Df:TM\rightarrow TN}

.

The tangent bundle comes equipped with a natural topology (not the disjoint union topology) and smooth structure so as to make it into a manifold in its own right. The dimension of

    T
    M
  

{\displaystyle TM}

is twice the dimension of

    M
  

{\displaystyle M}

.

Each tangent space of an n-dimensional manifold is an n-dimensional vector space. If

    U
  

{\displaystyle U}

is an open contractible subset of

    M
  

{\displaystyle M}

, then there is a diffeomorphism

    T
    U
    →
    U
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle TU\to U\times \mathbb {R} ^{n}}

which restricts to a linear isomorphism from each tangent space

      T
      
        x
      
    
    U
  

{\displaystyle T_{x}U}

to

    {
    x
    }
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle \{x\}\times \mathbb {R} ^{n}}

. As a manifold, however,

    T
    M
  

{\displaystyle TM}

is not always diffeomorphic to the product manifold

    M
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle M\times \mathbb {R} ^{n}}

. When it is of the form

    M
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle M\times \mathbb {R} ^{n}}

, then the tangent bundle is said to be trivial. Trivial tangent bundles usually occur for manifolds equipped with a 'compatible group structure'; for instance, in the case where the manifold is a Lie group. The tangent bundle of the unit circle is trivial because it is a Lie group (under multiplication and its natural differential structure). It is not true however that all spaces with trivial tangent bundles are Lie groups; manifolds which have a trivial tangent bundle are called parallelizable. Just as manifolds are locally modeled on Euclidean space, tangent bundles are locally modeled on

    U
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle U\times \mathbb {R} ^{n}}

, where

    U
  

{\displaystyle U}

is an open subset of Euclidean space.

If M is a smooth n-dimensional manifold, then it comes equipped with an atlas of charts

    (
    
      U
      
        α
      
    
    ,
    
      ϕ
      
        α
      
    
    )
  

{\displaystyle (U_{\alpha },\phi _{\alpha })}

, where

      U
      
        α
      
    
  

{\displaystyle U_{\alpha }}

is an open set in

    M
  

{\displaystyle M}

and

ϕ

        α
      
    
    :
    
      U
      
        α
      
    
    →
    
      
        R
      
      
        n
      
    
  

{\displaystyle \phi _{\alpha }:U_{\alpha }\to \mathbb {R} ^{n}}

is a diffeomorphism. These local coordinates on

      U
      
        α
      
    
  

{\displaystyle U_{\alpha }}

give rise to an isomorphism

      T
      
        x
      
    
    M
    →
    
      
        R
      
      
        n
      
    
  

{\displaystyle T_{x}M\rightarrow \mathbb {R} ^{n}}

for all

    x
    ∈
    
      U
      
        α
      
    
  

{\displaystyle x\in U_{\alpha }}

. We may then define a map

ϕ ~

        α
      
    
    :
    
      π
      
        −
        1
      
    
    
      (
      
        U
        
          α
        
      
      )
    
    →
    
      
        R
      
      
        2
        n
      
    
  

{\displaystyle {\widetilde {\phi }}_{\alpha }:\pi ^{-1}\left(U_{\alpha }\right)\to \mathbb {R} ^{2n}}

by

ϕ ~

        α
      
    
    
      (
      
        x
        ,
        
          v
          
            i
          
        
        
          ∂
          
            i
          
        
      
      )
    
    =
    
      (
      
        
          ϕ
          
            α
          
        
        (
        x
        )
        ,
        
          v
          
            1
          
        
        ,
        ⋯
        ,
        
          v
          
            n
          
        
      
      )
    
  

{\displaystyle {\widetilde {\phi }}_{\alpha }\left(x,v^{i}\partial _{i}\right)=\left(\phi _{\alpha }(x),v^{1},\cdots ,v^{n}\right)}

We use these maps to define the topology and smooth structure on

    T
    M
  

{\displaystyle TM}

. A subset

    A
  

{\displaystyle A}

of

    T
    M
  

{\displaystyle TM}

is open if and only if

ϕ ~

        α
      
    
    
      (
      
        A
        ∩
        
          π
          
            −
            1
          
        
        
          (
          
            U
            
              α
            
          
          )
        
      
      )
    
  

{\displaystyle {\widetilde {\phi }}_{\alpha }\left(A\cap \pi ^{-1}\left(U_{\alpha }\right)\right)}

is open in

        R
      
      
        2
        n
      
    
  

{\displaystyle \mathbb {R} ^{2n}}

for each

    α
    .
  

{\displaystyle \alpha .}

These maps are homeomorphisms between open subsets of

    T
    M
  

{\displaystyle TM}

and

        R
      
      
        2
        n
      
    
  

{\displaystyle \mathbb {R} ^{2n}}

and therefore serve as charts for the smooth structure on

    T
    M
  

{\displaystyle TM}

. The transition functions on chart overlaps

      π
      
        −
        1
      
    
    
      (
      
        
          U
          
            α
          
        
        ∩
        
          U
          
            β
          
        
      
      )
    
  

{\displaystyle \pi ^{-1}\left(U_{\alpha }\cap U_{\beta }\right)}

are induced by the Jacobian matrices of the associated coordinate transformation and are therefore smooth maps between open subsets of

        R
      
      
        2
        n
      
    
  

{\displaystyle \mathbb {R} ^{2n}}

.

The tangent bundle is an example of a more general construction called a vector bundle (which is itself a specific kind of fiber bundle). Explicitly, the tangent bundle to an

    n
  

{\displaystyle n}

-dimensional manifold

    M
  

{\displaystyle M}

may be defined as a rank

    n
  

{\displaystyle n}

vector bundle over

    M
  

{\displaystyle M}

whose transition functions are given by the Jacobian of the associated coordinate transformations.

The simplest example is that of

        R
      
      
        n
      
    
  

{\displaystyle \mathbb {R} ^{n}}

. In this case the tangent bundle is trivial: each

      T
      
        x
      
    
    
      
        
          R
        
      
      
        n
      
    
  

{\displaystyle T_{x}\mathbf {\mathbb {R} } ^{n}}

is canonically isomorphic to

      T
      
        
          0
        
      
    
    
      
        R
      
      
        n
      
    
  

{\displaystyle T_{\mathbf {0} }\mathbb {R} ^{n}}

via the map

        R
      
      
        n
      
    
    →
    
      
        R
      
      
        n
      
    
  

{\displaystyle \mathbb {R} ^{n}\to \mathbb {R} ^{n}}

which subtracts

    x
  

{\displaystyle x}

, giving a diffeomorphism

    T
    
      
        R
      
      
        n
      
    
    →
    
      
        R
      
      
        n
      
    
    ×
    
      
        R
      
      
        n
      
    
  

{\displaystyle T\mathbb {R} ^{n}\to \mathbb {R} ^{n}\times \mathbb {R} ^{n}}

.

Another simple example is the unit circle,

      S
      
        1
      
    
  

{\displaystyle S^{1}}

(see picture above). The tangent bundle of the circle is also trivial and isomorphic to

      S
      
        1
      
    
    ×
    
      R
    
  

{\displaystyle S^{1}\times \mathbb {R} }

. Geometrically, this is a cylinder of infinite height.

The only tangent bundles that can be readily visualized are those of the real line

      R
    
  

{\displaystyle \mathbb {R} }

and the unit circle

      S
      
        1
      
    
  

{\displaystyle S^{1}}

, both of which are trivial. For 2-dimensional manifolds the tangent bundle is 4-dimensional and hence difficult to visualize.

A simple example of a nontrivial tangent bundle is that of the unit sphere

      S
      
        2
      
    
  

{\displaystyle S^{2}}

: this tangent bundle is nontrivial as a consequence of the hairy ball theorem. Therefore, the sphere is not parallelizable.

A smooth assignment of a tangent vector to each point of a manifold is called a vector field. Specifically, a vector field on a manifold

    M
  

{\displaystyle M}

is a smooth map

V : M → T M

{\displaystyle V\colon M\to TM}

such that

    V
    (
    x
    )
    =
    (
    x
    ,
    
      V
      
        x
      
    
    )
  

{\displaystyle V(x)=(x,V_{x})}

with

      V
      
        x
      
    
    ∈
    
      T
      
        x
      
    
    M
  

{\displaystyle V_{x}\in T_{x}M}

for every

    x
    ∈
    M
  

{\displaystyle x\in M}

. In the language of fiber bundles, such a map is called a section. A vector field on

    M
  

{\displaystyle M}

is therefore a section of the tangent bundle of

    M
  

{\displaystyle M}

.

The set of all vector fields on

    M
  

{\displaystyle M}

is denoted by

    Γ
    (
    T
    M
    )
  

{\displaystyle \Gamma (TM)}

. Vector fields can be added together pointwise

( V + W

      )
      
        x
      
    
    =
    
      V
      
        x
      
    
    +
    
      W
      
        x
      
    
  

{\displaystyle (V+W)_{x}=V_{x}+W_{x}}

and multiplied by smooth functions on M

( f V

      )
      
        x
      
    
    =
    f
    (
    x
    )
    
      V
      
        x
      
    
  

{\displaystyle (fV)_{x}=f(x)V_{x}}

to get other vector fields. The set of all vector fields

    Γ
    (
    T
    M
    )
  

{\displaystyle \Gamma (TM)}

then takes on the structure of a module over the commutative algebra of smooth functions on M, denoted

      C
      
        ∞
      
    
    (
    M
    )
  

{\displaystyle C^{\infty }(M)}

.

A local vector field on

    M
  

{\displaystyle M}

is a local section of the tangent bundle. That is, a local vector field is defined only on some open set

    U
    ⊂
    M
  

{\displaystyle U\subset M}

and assigns to each point of

    U
  

{\displaystyle U}

a vector in the associated tangent space. The set of local vector fields on

    M
  

{\displaystyle M}

forms a structure known as a sheaf of real vector spaces on

    M
  

{\displaystyle M}

.

The above construction applies equally well to the cotangent bundle – the differential 1-forms on

    M
  

{\displaystyle M}

are precisely the sections of the cotangent bundle

    ω
    ∈
    Γ
    (
    
      T
      
        ∗
      
    
    M
    )
  

{\displaystyle \omega \in \Gamma (T^{*}M)}

,

    ω
    :
    M
    →
    
      T
      
        ∗
      
    
    M
  

{\displaystyle \omega :M\to T^{*}M}

that associate to each point

    x
    ∈
    M
  

{\displaystyle x\in M}

a 1-covector

      ω
      
        x
      
    
    ∈
    
      T
      
        x
      
      
        ∗
      
    
    M
  

{\displaystyle \omega _{x}\in T_{x}^{*}M}

, which map tangent vectors to real numbers:

      ω
      
        x
      
    
    :
    
      T
      
        x
      
    
    M
    →
    
      R
    
  

{\displaystyle \omega _{x}:T_{x}M\to \mathbb {R} }

. Equivalently, a differential 1-form

    ω
    ∈
    Γ
    (
    
      T
      
        ∗
      
    
    M
    )
  

{\displaystyle \omega \in \Gamma (T^{*}M)}

maps a smooth vector field

    X
    ∈
    Γ
    (
    T
    M
    )
  

{\displaystyle X\in \Gamma (TM)}

to a smooth function

    ω
    (
    X
    )
    ∈
    
      C
      
        ∞
      
    
    (
    M
    )
  

{\displaystyle \omega (X)\in C^{\infty }(M)}

.

Since the tangent bundle

    T
    M
  

{\displaystyle TM}

is itself a smooth manifold, the second-order tangent bundle can be defined via repeated application of the tangent bundle construction:

T

        2
      
    
    M
    =
    T
    (
    T
    M
    )
    .
    
  

{\displaystyle T^{2}M=T(TM).\,}

In general, the

    k
  

{\displaystyle k}

th order tangent bundle

      T
      
        k
      
    
    M
  

{\displaystyle T^{k}M}

can be defined recursively as

    T
    
      (
      
        
          T
          
            k
            −
            1
          
        
        M
      
      )
    
  

{\displaystyle T\left(T^{k-1}M\right)}

.

A smooth map

    f
    :
    M
    →
    N
  

{\displaystyle f:M\rightarrow N}

has an induced derivative, for which the tangent bundle is the appropriate domain and range

    D
    f
    :
    T
    M
    →
    T
    N
  

{\displaystyle Df:TM\rightarrow TN}

. Similarly, higher-order tangent bundles provide the domain and range for higher-order derivatives

      D
      
        k
      
    
    f
    :
    
      T
      
        k
      
    
    M
    →
    
      T
      
        k
      
    
    N
  

{\displaystyle D^{k}f:T^{k}M\to T^{k}N}

.

A distinct but related construction are the jet bundles on a manifold, which are bundles consisting of jets.

On every tangent bundle

    T
    M
  

{\displaystyle TM}

, considered as a manifold itself, one can define a canonical vector field

    V
    :
    T
    M
    →
    
      T
      
        2
      
    
    M
  

{\displaystyle V:TM\rightarrow T^{2}M}

as the diagonal map on the tangent space at each point. This is possible because the tangent space of a vector space W is naturally a product,

    T
    W
    ≅
    W
    ×
    W
    ,
  

{\displaystyle TW\cong W\times W,}

since the vector space itself is flat, and thus has a natural diagonal map

    W
    →
    T
    W
  

{\displaystyle W\to TW}

given by

    w
    ↦
    (
    w
    ,
    w
    )
  

{\displaystyle w\mapsto (w,w)}

under this product structure. Applying this product structure to the tangent space at each point and globalizing yields the canonical vector field. Informally, although the manifold

    M
  

{\displaystyle M}

is curved, each tangent space at a point

    x
  

{\displaystyle x}

,

      T
      
        x
      
    
    M
    ≈
    
      
        R
      
      
        n
      
    
  

{\displaystyle T_{x}M\approx \mathbb {R} ^{n}}

, is flat, so the tangent bundle manifold

    T
    M
  

{\displaystyle TM}

is locally a product of a curved

    M
  

{\displaystyle M}

and a flat

        R
      
      
        n
      
    
    .
  

{\displaystyle \mathbb {R} ^{n}.}

Thus the tangent bundle of the tangent bundle is locally (using

    ≈
  

{\displaystyle \approx }

for "choice of coordinates" and

    ≅
  

{\displaystyle \cong }

for "natural identification"):

T ( T M ) ≈ T ( M ×

        R
      
      
        n
      
    
    )
    ≅
    T
    M
    ×
    T
    (
    
      
        R
      
      
        n
      
    
    )
    ≅
    T
    M
    ×
    (
    
      
        R
      
      
        n
      
    
    ×
    
      
        R
      
      
        n
      
    
    )
  

{\displaystyle T(TM)\approx T(M\times \mathbb {R} ^{n})\cong TM\times T(\mathbb {R} ^{n})\cong TM\times (\mathbb {R} ^{n}\times \mathbb {R} ^{n})}

and the map

    T
    T
    M
    →
    T
    M
  

{\displaystyle TTM\to TM}

is the projection onto the first coordinates:

( T M → M ) × (

        R
      
      
        n
      
    
    ×
    
      
        R
      
      
        n
      
    
    →
    
      
        R
      
      
        n
      
    
    )
    .
  

{\displaystyle (TM\to M)\times (\mathbb {R} ^{n}\times \mathbb {R} ^{n}\to \mathbb {R} ^{n}).}

Splitting the first map via the zero section and the second map by the diagonal yields the canonical vector field.

If

    (
    x
    ,
    v
    )
  

{\displaystyle (x,v)}

are local coordinates for

    T
    M
  

{\displaystyle TM}

, the vector field has the expression

V =

      ∑
      
        i
      
    
    
      
        
        
          
            v
            
              i
            
          
          
            
              ∂
              
                ∂
                
                  v
                  
                    i
                  
                
              
            
          
        
        |
      
      
        (
        x
        ,
        v
        )
      
    
    .
  

{\displaystyle V=\sum _{i}\left.v^{i}{\frac {\partial }{\partial v^{i}}}\right|_{(x,v)}.}

More concisely,

    (
    x
    ,
    v
    )
    ↦
    (
    x
    ,
    v
    ,
    0
    ,
    v
    )
  

{\displaystyle (x,v)\mapsto (x,v,0,v)}

– the first pair of coordinates do not change because it is the section of a bundle and these are just the point in the base space: the last pair of coordinates are the section itself. This expression for the vector field depends only on

    v
  

{\displaystyle v}

, not on

    x
  

{\displaystyle x}

, as only the tangent directions can be naturally identified.

Alternatively, consider the scalar multiplication function:

{

                R
              
              ×
              T
              M
              →
              T
              M
            
          
          
            
              (
              t
              ,
              v
              )
              ⟼
              t
              v
            
          
        
        
      
    
  

{\displaystyle {\begin{cases}\mathbb {R} \times TM\to TM\\(t,v)\longmapsto tv\end{cases}}}

The derivative of this function with respect to the variable

      R
    
  

{\displaystyle \mathbb {R} }

at time

    t
    =
    1
  

{\displaystyle t=1}

is a function

    V
    :
    T
    M
    →
    
      T
      
        2
      
    
    M
  

{\displaystyle V:TM\rightarrow T^{2}M}

, which is an alternative description of the canonical vector field.

The existence of such a vector field on

    T
    M
  

{\displaystyle TM}

is analogous to the canonical one-form on the cotangent bundle. Sometimes

    V
  

{\displaystyle V}

is also called the Liouville vector field, or radial vector field. Using

    V
  

{\displaystyle V}

one can characterize the tangent bundle. Essentially,

    V
  

{\displaystyle V}

can be characterized using 4 axioms, and if a manifold has a vector field satisfying these axioms, then the manifold is a tangent bundle and the vector field is the canonical vector field on it. See for example, De León et al.

There are various ways to lift objects on

    M
  

{\displaystyle M}

into objects on

    T
    M
  

{\displaystyle TM}

. For example, if

    γ
  

{\displaystyle \gamma }

is a curve in

    M
  

{\displaystyle M}

, then

      γ
      ′
    
  

{\displaystyle \gamma '}

(the tangent of

    γ
  

{\displaystyle \gamma }

) is a curve in

    T
    M
  

{\displaystyle TM}

. In contrast, without further assumptions on

    M
  

{\displaystyle M}

(say, a Riemannian metric), there is no similar lift into the cotangent bundle.

The vertical lift of a function

    f
    :
    M
    →
    
      R
    
  

{\displaystyle f:M\rightarrow \mathbb {R} }

is the function

      f
      
        ∨
      
    
    :
    T
    M
    →
    
      R
    
  

{\displaystyle f^{\vee }:TM\rightarrow \mathbb {R} }

defined by

      f
      
        ∨
      
    
    =
    f
    ∘
    π
  

{\displaystyle f^{\vee }=f\circ \pi }

, where

    π
    :
    T
    M
    →
    M
  

{\displaystyle \pi :TM\rightarrow M}

is the canonical projection.

  • Pushforward (differential)
  • Unit tangent bundle
  • Cotangent bundle
  • Frame bundle
  • Musical isomorphism
  • Holomorphic tangent bundle
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This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed.Find sources: "Tangent bundle" – news · newspapers · books · scholar · JSTOR (July 2009) (Learn how and when to remove this message)
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  • Lee, John M. (2012). Introduction to Smooth Manifolds. Graduate Texts in Mathematics. Vol. 218. doi:10.1007/978-1-4419-9982-5. ISBN 978-1-4419-9981-8.

  • Jürgen Jost, Riemannian Geometry and Geometric Analysis, (2002) Springer-Verlag, Berlin. ISBN 3-540-42627-2

  • Ralph Abraham and Jerrold E. Marsden, Foundations of Mechanics, (1978) Benjamin-Cummings, London. ISBN 0-8053-0102-X

  • León, M. De; Merino, E.; Oubiña, J. A.; Salgado, M. (1994). "A characterization of tangent and stable tangent bundles" (PDF). Annales de l'I.H.P.: Physique Théorique. 61 (1): 1–15.

  • Gudmundsson, Sigmundur; Kappos, Elias (2002). "On the geometry of tangent bundles". Expositiones Mathematicae. 20: 1–41. doi:10.1016/S0723-0869(02)80027-5.

  • Salimov, Arif (2023). Applications of Holomorphic Functions in Geometry. Frontiers in Mathematics, Birkhäuser. doi:10.1007/978-981-99-1296-4. ISBN 978-1-4419-9981-8.

  • "Tangent bundle", Encyclopedia of Mathematics, EMS Press, 2001 [1994]

  • Wolfram MathWorld: Tangent Bundle

  • PlanetMath: Tangent Bundle

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