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In Mathematics a vector field is a construction in Vector Calculus which associates a Vector to every point in a (locally) Euclidean Space .

Vector fields are often used in Physics to model, for example, the speed and direction of a moving fluid throughout space, or the strength and direction of some Force , such as the Magnetic or Gravitational force, as it changes from point to point.

In the rigorous mathematical treatment, (tangent) vector fields are defined on Manifold s as Section s of a manifold's Tangent Bundle . They are one kind of Tensor Field on the manifold.


DEFINITION



Vector fields on subsets of Euclidean space

Given a subset ''S'' in R''n'', a '''vector field''' is represented by a Vector-valued Function
V_x: S o \mathbf{R}^n
in standard Euclidean coordinates (''x''1, ..., ''x''''n''). If there is another coordinate system ''y'' on ''S'', then
V_y := rac{\partial y}{\partial x} V_x
is the expression for the same vector field in the new coordinates ''y''. In particular, a vector field is not just a collection of Scalar Fields .

We say ''V'' is a C''k'' vector field if ''V'' is ''k'' times Continuously Differentiable . A point ''p'' in ''S'' is called stationary if the vector at that point is zero
(V(p) = 0).

A vector field can be visualized as a ''n''-dimensional space with a ''n''-dimensional vector attached to each point.
Given two C''k''-vector fields ''V'', ''W'' defined on ''S'' and a real valued C''k''-function ''f'' defined on ''S'', the two operations scalar multiplication and vector addition

: (fV)(p) := f(p)V(p)

: (V+W)(p) := V(p) + W(p)

define the Module of C''k''-vector fields over the Ring of C''k''-functions.


Vector fields on manifolds

.]]
Given a Manifold ''M'', a vector field on ''M'' is an assignment to every point of ''M'' a Tangent Vector to ''M'' at that point. That is, for each ''x'' in ''M'', we have a tangent vector ''v''(''x'') in T''x''''M''. More abstractly, a vector field is a Section of the Tangent Bundle T''M''. If this section is continuous/differentiable/smooth/analytic, then we call the vector field continuous/differentiable/smooth/analytic.

The collection of all vector fields on ''M'' is often denoted by Γ(T''M'') or ''C''∞(''M'',T''M'') (especially when thinking of vector fields as sections); the collection of all smooth vector fields is sometimes also denoted by \mathfrak{X} (M) (a Fraktur "X").


NOTES


Vector fields should be compared to Scalar Field s, which associate a number or ''scalar'' to every point in space (or every point of some manifold). Vector fields similarly associate a length or ''magnitude'', as well as a ''direction'' to every point in space. For example, in the common (x,y,z) three-space, every point in the manifold can be associated parametrically with magnitudes of x, y and z components.

The Divergence and Curl are two operations on a vector field which result in a scalar field and another vector field respectively. The first of these operations is defined in any number of dimensions (that is, for any value of ''n''). The curl however, is defined only for ''n''=3, but it can be generalized to an arbitrary dimension using the Exterior Product and Exterior Derivative .


EXAMPLES

s showing a Wingtip Vortex .]]
  • A vector field for the movement of air on Earth will associate for every point on the surface of the Earth a vector with the wind speed and direction for that point. This can be drawn using arrows to represent the wind; the length ( Magnitude ) of the arrow will be an indication of the wind speed. A "high" on the usual Barometric Pressure map would then act as a source (arrows pointing away), and a "low" would be a sink (arrows pointing towards), since air tends to move from high pressure areas to low pressure areas.

  • Velocity field of a moving Fluid . In this case, a Velocity vector is associated to each point in the fluid.

  • Streamlines, Streaklines And Pathlines are 3 types of lines that can be made from vector fields. They are :

    • ::streaklines — as revealed in Wind Tunnel s using smoke.

::streamlines (or fieldlines)— as a line depicting the instantaneous field at a given time.
::pathlines — showing the path that a given particle (of zero mass) would follow.
  • Magnetic Field s. The fieldlines can be revealed using small Iron filings.

  • Maxwell's Equations allow us to use a given set of initial conditions to deduce, for every point in Euclidean Space , a magnitude and direction for the Force experienced by a charged test particle at that point; the resulting vector field is the Electromagnetic Field .

  • A Gravitational Field generated by any massive object is also a vector field. For example, field lines for a spherically symmetric body would all point towards the sphere's center with the magnitude of the field lines reducing as radial distance from the body increases.



Gradient field


Vector fields can be constructed out of Scalar Field s using the vector operator Gradient which gives rise to the following definition.

A vector field ''V'' defined on a set ''S'' is called a gradient field or a '''conservative field''' if there exists a real valued function (a scalar field) ''f'' on ''S'' such that

:V =
abla f.

The path integral along any closed curve γ (γ(0) = γ(1)) in a gradient field is zero:
: \int_\gamma \langle V(x), \mathrm{d}x angle = \int_\gamma \langle
abla f(x), \mathrm{d}x angle = f(\gamma(1)) - f(\gamma(0)).


Central field


A ''C''∞-vector field over R''n'' \ {0} is called a '''central field''' if

:V(T(p)) = T(V(p)) \qquad (T \in \mathrm{O}(n, \mathbf{R}))

where O(''n'', R) is the Orthogonal Group . We say central fields are Invariant under Orthogonal Transformations around 0.

The point 0 is called the center of the field.

Since orthogonal transformations are actually rotations and reflections, the invariance conditions mean that vectors of a central field are always directed towards, or away from, 0; this is an alternate (and simpler) definition.
A central field is always a gradient field, since defining it on one semiaxis and integrating gives an antigradient.


CURVE INTEGRAL


A common technique in physics is to integrate a vector field along a . Given a particle in a gravitational vector field, where each vector represents the force acting on the particle at this point in space, the curve integral is the work done on the particle when it travels along a certain path.

The curve integral is constructed analogously to the Riemann Integral and it exists if the curve is rectifiable (has finite length) and the vector field is continuous.

Given a vector field ''V'' and a curve γ parametrized by 1 the curve integral is defined as

:\int_\gamma \langle V(x), \mathrm{d}x angle = \int_0^1 \langle V(\gamma(t)), \gamma'(t)\;\mathrm{d}t angle.



FLOW CURVES


Vector fields have a nice interpretation in terms of autonomous, first order Ordinary Differential Equation s.

Given a vector field ''V'' defined on ''S'', we can try to define curves γ on ''S'' such that for each ''t'' in an interval ''I''

:\gamma'(t) = V(\gamma(t))

If ''V'' is Lipschitz Continuous we can find a unique ''C''1-curve γ''x'' for each point ''x'' in ''S'' so that
:\gamma_x(0) = x
:\gamma'_x(t) = V(\gamma_x(t)) \qquad ( t \in (-\epsilon, +\epsilon) \subset \mathbf{R})

The curves γ''x'' are called flow curves of the vector field ''V'' and partition ''S'' into Equivalence Class es. It is not always possible to extend the interval (-ε, +ε) to the whole Real Number Line . The flow may for example reach the edge of ''S'' in a finite time.



In two or three dimensions one can visualize the vector field as giving rise to a Flow on ''S''. If we drop a particle into this flow at a point ''p'' it will move along the curve γ''p'' in the flow depending on the initial point ''p''. If ''p'' is a stationary point of ''V'' then the particle will remain at ''p''.

Typical applications are Streamline in Fluid , Geodesic Flow , and One-parameter Subgroup s and the Exponential Map in Lie Group s.


DIFFERENCE BETWEEN SCALAR AND VECTOR FIELD


The difference between a scalar and vector field is not that a scalar is just one number while a vector is several numbers. The difference is in how their coordinates respond to coordinate transformations. A scalar ''is'' a coordinate whereas a vector ''can be described'' by coordinates, but it ''is not'' the collection of its coordinates.


Example 1

This example is about 2-dimensional Euclidean space (R2) where we examine Euclidean (''x'', ''y'') and Polar (''r'', θ) coordinates (which are undefined at the origin). Thus ''x'' = ''r'' cos θ and ''y'' = ''r'' sin θ and also ''r''2 = ''x''2 + ''y''2, cos θ = ''x''/(''x''2 + ''y''2)1/2 and sin θ = ''y''/(''x''2 + ''y''2)1/2. Suppose we have a scalar field which is given by the constant function 1, and a vector field which attaches a vector in the ''r''-direction with length 1 to each point. More precisely, they are given by the functions

:s_{\mathrm{polar}}:(r, heta) \mapsto 1, \quad v_{\mathrm{polar}}:(r, heta) \mapsto (1, 0).

Let us convert these fields to Euclidean coordinates. The vector of length 1 in the ''r''-direction has the ''x'' coordinate cos θ and the ''y'' coordinate sin θ. Thus in Euclidean coordinates the same fields are described by the functions

:s_{\mathrm{Euclidean}}:(x, y) \mapsto 1, \quad v_{\mathrm{Euclidean}}:(x, y) \mapsto (\cos heta, \sin heta) = \left( rac{x}\sqrt, rac{y}{\sqrt{x^2 + y^2}} ight).

We see that while the scalar field remains the same, the vector field now looks different. The same holds even in the 1-dimensional case, as illustrated by the next example.


Example 2

Consider the 1-dimensional Euclidean space R with its standard Euclidean coordinate ''x''. Suppose we have a scalar field and a vector field which are both given in the ''x'' coordinate by the constant function 1,

:s_{\mathrm{Euclidean}}:x \mapsto 1, \quad v_{\mathrm{Euclidean}}:x \mapsto 1.

Thus, we have a scalar field which has the value 1 everywhere and a vector field which attaches a vector in the ''x''-direction with magnitude 1 unit of ''x'' to each point.

Now consider the coordinate ξ := 2''x''. If ''x'' changes one unit then ξ changes 2 units. Thus this vector field has a magnitude of 2 in units of ξ. Therefore, in the ξ coordinate the scalar field and the vector field are described by the functions

:s_{\mathrm{unusual}}:\xi \mapsto 1, \quad v_{\mathrm{unusual}}:\xi \mapsto 2.

which are different.


SEE ALSO




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