13.6 Vector Fields

We begin with a quote of Jerold Marsden, Carl F. Braun distinguished Professor at Caltech and a fellow of the Royal Society.

The Field Concept

The concept of a “field,” such as a vector field, has had an enormous impact on the development of conceptual frameworks for physics and engineering. It is truly one of the great breakthrough ideas in the history of human thought. It is the notion that allows us to describe, in a systematic way, influences on objects and between objects that are spatially separated.

The idea of a field began with Newton’s concept of the gravitational field. In this case, the gravitational field describes the attractive influence of a group of bodies on each other. Similarly, the electric field produced by a charged object or group of objects creates, according to Coulomb’s law, a force on another charged object. Using vector fields to describe these sorts of forces has led to a deeper understanding of attractive and repulsive forces in nature.

However, it was the monumental discovery of the Maxwell field equations, which describe the propagation of electromagnetic energy, that cemented the concept of “field” in scientific thought. This example is particularly interesting because these fields can propagate. The contrast between the electromagnetic field that can propagate and the gravitational field that involves instantaneous action at a distance has caused great interest among philosophers of science.

Einstein’s idea is that gravitation can be described in terms of the metric properties of space–time and that in this theory the associated field can also propagate, just like the electromagnetic field, thus providing profound philosophical evidence that Einstein’s version of gravity may be correct. These ideas have also led to modern efforts to detect gravitational waves. For a further discussion of Einstein’s work, see Section 17.7.

The idea of a field is also used in engineering to describe elastic systems and interesting microstructural properties of materials. In modern theoretical physics, the field concept is used to describe elementary particles and is central to attempts by modern theoretical physicists to unify gravity with the quantum mechanical physics of elementary particles. It is impossible to imagine a modern theoretical framework that does not incorporate some sort of field concept as a central ingredient.

The Concept of a Vector Field

In Section 13.5 we introduced a particular kind of vector field, the gradient. In this section we study general vector fields, discussing their geometric and physical significance.

Picture \({\bf F}\) as attaching an arrow to each point (Figure 13.55). By contrast, a map \(f\colon A\subset {\mathbb R}^n \rightarrow {\mathbb R}\) that assigns a number to each point is a scalar field. A vector field \({\bf F}(x,y,z)\) on \({\mathbb R}^3\) has three component scalar fields \(F_1,F_2\), and \(F_3\), so that \[ {\bf F}(x,y,z)=(F_1(x,y,z),F_2 (x,y,z),F_3(x,y,z)). \]

Similarly, a vector field on \({\mathbb R}^n\) has \(n\) components \(F_1,\ldots ,F_n\). If each component is a \(C^k\) function, we say the vector field \({\bf F}\) is of class \(C^k\). Vector fields will be assumed to be at least of class \(C^1\) unless otherwise noted. In many applications, \({\bf F}({\bf x})\) represents a physical vector quantity (force, velocity, etc.) associated with the position \({\bf x}\), as in the following examples.

Gradient Vector Fields

In Section 13.3 we introduced the gradient of a function by \[ \nabla f(x,y,z)=\frac{\partial f}{\partial x}(x,y,z){\bf i}+\frac{\partial f}{\partial y}(x,y,z){\bf j}+\frac{\partial f}{\partial z}(x,y,z){\bf k}. \]

Now we want to think of this as an example of a vector field—it assigns a vector to each point (\(x, y, z\)). As such, we refer to \(\nabla f\) as a gradient vector field. Gradient fields come up in a variety of situations, as the next two examples show.

The next example shows that not every vector field is a gradient.

Conservation of Energy and Escaping the Earth’s Gravitational Field

Consider a particle of mass \(m\) moving in a force field \({\bf F}\) that is a potential field. That is, assume \({\bf F}\,{=}\,{-}\nabla V\) for a real-valued function \(V\), and that the particle moves according to \({\bf F}\,{=}\,m{\bf a}\). Thus, if the path is \({\bf r}(t)\), then \begin{equation} m\ddot{\bf r}(t) = {-}\nabla V({\bf r}(t)). \end{equation}

A basic fact about such motion is the conservation of energy. The energy \(E\) of the particle is defined to be the sum of the kinetic and potential energies, defined as \begin{equation} E=\frac{1}{2}m\|\dot{\bf r}(t)\|^2+V({\bf r}(t)). \end{equation}

The principle of conservation of energy states that if Newton’s second law holds, then \(E\) is independent of time; that is, \({\it dE}{/}{\it dt}\,{=}\,0\). The proof of this fact is a simple calculation; we use equation (2), the chain rule, and equation (1): \begin{eqnarray*} \frac{{\it dE}}{{\it dt}} &=& m\dot{\bf r}\,{\cdot}\,\ddot{\bf r}+(\nabla V)\,{\cdot}\,\dot{\bf r}\\[4pt] &=&\dot{\bf r}\,{\cdot}\,(-\nabla V+\nabla V)=0. \end{eqnarray*}

Escape Velocity

As an application of conservation of energy, we compute the velocity required for a rocket to escape the earth's gravitational influence. Assume the rocket has mass \(m\) and is at a distance \(R_{0}\) from the center of the earth (or another planet) when its escape velocity \(v_{e}\) has been reached, and that it will coast thereafter. The energy at this time is \begin{equation} E_0=\frac{1}{2}mv^2_e - \frac{m{\it MG}}{R_0}. \end{equation}

By conservation of energy, \(E_{0}\) will equal the energy at a later time, which we write as \begin{equation} E_0=E=\frac{1}{2}mv^2 - \frac{m{\it MG}}{R}, \end{equation} where \(v\) is the velocity and \(R\) is the distance from the center of the earth (or the other planet). What we mean by the term escape velocity is that \(v_{e}\) is chosen such that the rocket gets to great distances, at which time it is barely moving. That is, \(v\) is close to zero and \(R\) is very large. Thus, from equation (4), we see that \(E = 0\) and hence \(E_{0} = 0\); solving \(E_{0} = 0\) for \(v_{e}\) using equation (3) gives: \[ v_e = \sqrt{\frac{2{\it MG}}{R_0}}. \]

Now \({\it GM}/R^{2}_{0}\) is exactly \(g\), the acceleration due to gravity at the distance \(R_{0}\) from the center of the planet. Thus, we can write: \[ v_e=\sqrt{2gR_0}. \]

For the earth, if the escape velocity were to be achieved at the surface of the earth (of course, this is a bit unrealistic), this would give \[ v_e=\sqrt{2\,{\cdot}\,9.8 \ {\rm m\hbox{/}s}^2{\cdot}\,\hbox{6,371,000} \ {\rm m}}=\hbox{11,127} \ {\rm m\hbox{/}s}. \]

However, this is a good approximation to the velocity that a satellite in low earth orbit needs in order to escape the earth’s gravitational field.

Flow Lines

An important concept related to general (not necessarily gradient) vector fields is that of a flow line, defined as follows.

In the context of Example 1, a flow line is the path followed by a small particle suspended in the fluid (Figure 13.62). Flow lines are also appropriately called streamlines or integral curves.

Geometrically, a flow line for a given vector filed \({\bf F}\) is a curve that threads its way through the domain of the vector field in such a way that the tangent vector of the curve coincides with the vector field, as in Figure 13.63.

A flow line may be viewed as a solution of a system of differential equations. Indeed, we can write the definition \({\bf c}'(t)={\bf F}({\bf c}(t))\) as \begin{eqnarray*} x'(t) &=& P(x(t),y(t),z(t)),\\[3pt] y'(t) &=& Q(x(t),y(t),z(t)),\\[3pt] z'(t) &=& R(x(t),y(t),z(t)), \end{eqnarray*} where \({\bf c}(t)=x(t){\bf i}+y(t){\bf j}+z(t){\bf k}\), and where \[ {\bf F}=P{\bf i}+Q{\bf j}+R{\bf k}. \]

You probably learned about such systems in courses on differential equations, but we are not presuming such a course has been taken.

In many cases, explicit formulas for flow lines are not available, so we must resort to numerical methods. Figure 13.64 shows some output from a program that computes flow lines numerically and plots them on the screen.