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Show that if \(f\) and \(g\) are scalars having continuous second partial derivatives in a domain \(D\), then $$ \mathbf{u}=\boldsymbol{\nabla} f \times \nabla g $$ is solenoidal in \(D\). (It can be shown that every solenoidal vector has such a reprefentation, at least in a suitably restricted domain.)

Short Answer

Expert verified
Question: Show that the vector field \(\mathbf{u}\) given by \(\mathbf{u}=\nabla f \times \nabla g\) is solenoidal in the domain \(D\). Answer: The divergence of \(\mathbf{u}\) is zero in \(D\), so \(\mathbf{u}\) is solenoidal.

Step by step solution

01

Calculate the cross product of the gradients

First, let's calculate the vector field \(\mathbf{u}\), which is defined as the cross product of the gradients of \(f\) and \(g\). $$ \mathbf{u} = \nabla f \times \nabla g $$
02

Calculate the curl of the gradients

In order to use the first identity mentioned above, we need to calculate the curl of the gradients of \(f\) and \(g\). $$ \nabla \times (\nabla f) = \mathbf{0} $$ $$ \nabla \times (\nabla g) = \mathbf{0} $$ Note that the curl of the gradient of any scalar field is always zero.
03

Apply the identity

Now that we know the curl of the gradients, we can use the identity mentioned above to calculate the divergence of the cross product of the gradients. $$ \nabla \cdot \mathbf{u} = \nabla \cdot (\nabla f \times \nabla g) = \nabla g \cdot (\nabla \times \nabla f) - \nabla f \cdot (\nabla \times \nabla g) $$
04

Plug in the curls and simplify

We now substitute the curls we calculated earlier and simplify the expression. $$ \nabla \cdot \mathbf{u} = \nabla g \cdot \mathbf{0} - \nabla f \cdot \mathbf{0} = 0 $$
05

Conclusion

Since the divergence of \(\mathbf{u}\) is zero for all points in the domain \(D\), it is a solenoidal vector field. This confirms that $$ \mathbf{u} = \nabla f \times \nabla g $$ is indeed solenoidal in \(D\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Cross Product of Gradients
In vector calculus, the cross product of gradients is a powerful tool used to create a vector field from two scalar functions. To compute the cross product of the gradients of two scalar functions, say \( f \) and \( g \), we first need to calculate their respective gradients, \( abla f \) and \( abla g \).

The gradient of a scalar function is essentially a vector that points in the direction of the steepest increase of the function. For a function \( f(x, y, z) \), the gradient is calculated as \( abla f = \left( \frac{\partial f}{\partial x}, \frac{\partial f}{\partial y}, \frac{\partial f}{\partial z} \right) \).
Similarly, \( abla g \) is the gradient of the function \( g(x, y, z) \).
  • To find the cross product \( \mathbf{u} = abla f \times abla g \), use the determinant of a matrix constructed from the unit vectors \( \mathbf{i}, \mathbf{j}, \mathbf{k} \), the components of \( abla f \), and \( abla g \).
  • This cross product \( \mathbf{u} \) is a vector field that is orthogonal to both \( abla f \) and \( abla g \).
Continuous Second Partial Derivatives
For scalar functions \( f \) and \( g \) to consistently define a vector field through their gradients, they are required to have continuous second partial derivatives in their domain \( D \).

Continuous second partial derivatives mean that all second-order derivatives of the functions are continuous in that domain. Mathematically, this means:
  • \( \frac{\partial^2 f}{\partial x^2} \), \( \frac{\partial^2 f}{\partial x\partial y} \), \( \frac{\partial^2 f}{\partial x\partial z} \), and so on, are continuous for \( f \).
  • Similarly continuous derivatives exist for \( g \).

The existence of continuous partial derivatives ensures that these functions are smooth, that helps avoid undefined gradient values at any point in the domain.
This property is crucial when applying theorems like Green's theorem or the Divergence theorem, which rely on smoothness for calculus operations.
Divergence
Divergence is an operator that measures the extent to which a vector field acts as a source or a sink at a given point.
For a vector field \( \mathbf{v} = (v_1, v_2, v_3) \), the divergence is calculated as \( abla \cdot \mathbf{v} = \frac{\partial v_1}{\partial x} + \frac{\partial v_2}{\partial y} + \frac{\partial v_3}{\partial z} \).

In context, for \( \mathbf{u} = abla f \times abla g \), we want to determine if \( \mathbf{u} \) is solenoidal, meaning it has zero divergence everywhere in \( D \).
With:
  • The property that the curl of any gradient is zero: \( abla \times abla f = \mathbf{0} \)
  • The identity \( abla \cdot (abla f \times abla g) = abla g \cdot (abla \times abla f) - abla f \cdot (abla \times abla g) \)
When you apply these, the divergence simplifies to zero, confirming the solenoidal nature of \( \mathbf{u} \).
Thus, \( \mathbf{u} \), having zero divergence everywhere in \( D \), does not act as a source or a sink.
Curl of a Gradient
The curl of a gradient is always a noteworthy concept in vector calculus because it simplifies many problems.
When we calculate the curl of the gradient of a scalar function \( f \), we get:
  • \( abla \times (abla f) = \mathbf{0} \)

This result holds because differentiation is commutative; hence the mixed second partial derivatives cancel each other out.

This property is instrumental in simplifying the problem of determining if a vector field like \( \mathbf{u} \) is solenoidal. Since \( \mathbf{u} = abla f \times abla g \) involves the curl of \( abla f \) and \( abla g \), both being zero, it leads directly to the conclusion that \( \mathbf{u} \) is solenoidal.
Understanding this concept saves a lot of time and computation in both theoretical and practical applications of vector calculus.

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Most popular questions from this chapter

(Degree of mapping of one surface into another) Let \(S_{w v w}\) and \(S_{x y z}\) be surfaces forming the boundaries of regions \(R_{u v w}\) and \(R_{x y z}\) respectively: it is assumed that \(R_{u v w}\) and \(R_{x y}\). are bounded and closed and that \(R_{x y z}\) is simply connected. Let \(S_{u v w}\) and \(S_{x y z}\) be oriented by the outer normal. Let \(s, t\) be parameters for \(S_{u v w}\) : $$ u=u(s, t), \quad v=v(s, t), \quad w=w(s, t), $$ the normal having the direction of $$ \left(u_{s} \mathbf{i}+v_{s} \mathbf{j}+w_{s} \mathbf{k}\right) \times\left(u_{\mathbf{i}} \mathbf{i}+v_{t} \mathbf{j}+w_{t} \mathbf{k}\right) $$ Let $$ x=x(u, v, w), \quad y=y(u, v, w), \quad z=z(u, v, w) $$ be functions defined and having continuous derivatives in a domain containing \(S_{u v w}\), an let these equations define a mapping of \(S_{u v w}\) into \(S_{x y z}\). The degree \(\delta\) of this mapping i defined as \(1 / 4 \pi\) times the solid angle \(\Omega(O, S)\) of the image \(S\) of \(S_{u v w}\) with respect t a point \(O\) interior to \(S_{x y z}\). If \(O\) is the origin, the degree is hence given by the integra (Kronecker integral) $$ \delta=\frac{1}{4 \pi} \iint_{R_{u t}}\left|\begin{array}{ccc} x & y & z \\ \frac{\partial x}{\partial s} & \frac{\partial y}{\partial s} & \frac{\partial z}{\partial s} \\ \frac{\partial x}{\partial t} & \frac{\partial y}{\partial t} & \frac{\partial z}{\partial t} \end{array}\right| \frac{1}{\left(x^{2}+y^{2}+z^{2}\right)^{\frac{1}{2}}} d s d t $$ where \(x, y, z\) are expressed in terms of \(s, t\) by (a) and (b). It can be shown that \(\delta\), as thu defined, is independent of the choice of the interior point \(O\), that \(\delta\) is a positive or negativ integer or zero, and that \(\delta\) does measure the effective number of times that \(S_{x y z}\) is covered Let \(S_{k v w}\) be the sphere \(u=\sin s \cos t, v=\sin s \sin t, w=\cos s, 0 \leq s \leq \pi, 0\) \(t \leq 2 \pi\). Let \(S_{x y z}\) be the sphere \(x^{2}+y^{2}+z^{2}=1\). Evaluate the degree for the followin; mappings of \(S_{u v w}\) into \(S_{x y z}\); a) \(x=v, y=-w, z=u\) b) \(x=u^{2}-v^{2}, y=2 u v, z=w \sqrt{2-w^{2}}\)

Show that on the basis of the laws of thermodynamics, the line integral $$ \int S d T+p d V $$ is independent of the path in the \(T V\) plane. The integrand is minus the differential of the free energy \(F\).

(The solid angle) Let \(S\) be a plane surface, oriented in accordance with a unit normal \(\mathbf{n}\). The solid angle \(\Omega\) of \(S\) with respect to a point \(O\) not in \(S\) is defined as $$ \Omega(O, S)=\pm \text { area of projection of } S \text { on } S_{1}, $$ where \(S_{1}\) is the sphere of radius 1 about \(O\) and the \(+\) or - sign is chosen according to whether \(\mathbf{n}\) points away from or toward the side of \(S\) on which \(O\) lies. This is suggested in Fig. 5.37. a) Show that if \(O\) lies in the plane of \(S\) but not in \(S\), then \(\Omega(O, S)=0\). it b) Show that if \(S\) is a complete (that is, infinite) plane, then \(\Omega(O, S)=\pm 2 \pi\). c) For a general oriented surface \(S\) the surface can be thought of as made up of small elements, each of which is approximately planar and has a normal \(\mathbf{n}\). Justify the following definition of element of solid angle for such a surface element: $$ d \Omega=\frac{\mathbf{r} \cdot \mathbf{n}}{r^{3}} d \sigma $$ where \(\mathbf{r}\) is the vector from \(O\) to the element. d) On the basis of the formula of (c), one obtains as solid angle for a general oriented surface \(S\) the integral $$ \Omega(O, S)=\iint_{S} \frac{\mathbf{r} \cdot \mathbf{n}}{r^{3}} d \sigma . $$ Show that for surfaces in parametric form, if \(O\) is the origin, $$ \Omega(O, S)=\iint_{R_{x r}}\left|\begin{array}{ccc} x & y & z \\ \frac{\partial x}{\partial u} & \frac{\partial y}{\partial u} & \frac{\partial z}{\partial u} \\ \frac{\partial x}{\partial v} & \frac{\partial y}{\partial v} & \frac{\partial z}{\partial v} \end{array}\right| \frac{1}{\left(x^{2}+y^{2}+z^{2}\right)^{\frac{1}{2}}} d u d v . $$ This formula permits one to define a solid angle for complicated surfaces that interac themselves. e) Show that if the normal of \(S_{1}\) is the outer one, then \(\Omega(O, S)=4 \pi\). f) Show that if \(S\) forms the boundary of a bounded, closed, simply connected region \(R\). then \(\Omega(O, S), \pm 4 \pi\), when \(O\) is inside \(S\) and \(\Omega(O, S)=0\) when \(O\) is outside \(S\). g) If \(S\) is a fixed circular disk and \(O\) is variable, show that \(-2 \pi \leq \Omega(O, S) \leq 2 \pi\) and that \(\Omega(O, S)\) jumps by \(4 \pi\) as \(O\) crosses \(S\).

Let \(D\) he a simply connected domain in the \(x y\)-plane and let \(\mathbf{w}=u \mathbf{i}-v \mathbf{j}\) be the velocity vector of an irrotational incompressible flow in \(D\). (This is the same as an irrotational incompressible flow in a 3-dimensional domain whose projection is \(D\) and for which the \(z\)-component of velocity is 0 whereas the \(x\) - and \(y\)-components of velocity are independent of \(z\).) Show that the following propertics hold: a) \(u\) and \(v\) satisfy the Cauchy-Riemann equations: $$ \frac{\partial u}{\partial x}=\frac{\partial v}{\partial y}, \quad \frac{\partial u}{\partial y}=-\frac{\partial v}{\partial x} \text { in } D ; $$ b) \(u\) and \(v\) are harmonic in \(D\); c) \(\int u d x-v d y\) and \(\int v d x+u d y\) are independent of the path in \(D\); d) there is a vector \(\mathbf{F}=\phi \mathbf{i}-\psi \mathbf{j}\) in \(D\) such that $$ \frac{\partial \phi}{\partial x}=u=\frac{\partial \psi}{\partial y}, \quad \frac{\partial \phi}{\partial y}=-v=-\frac{\partial \psi}{\partial x} ; $$ e) \(\operatorname{div} \mathbf{F}=0\) and curl \(\mathbf{F}=\mathbf{0}\) in \(D\); f) \(\phi\) and \(\psi\) are harmonic in \(D\); g) \(\operatorname{grad} \phi=\mathbf{w}, \psi\) is constant on each stream line. The function \(\phi\) is the velocity potential; \(\psi\) is the stream function.

Let a wire occupying the line segment from \((0,-c)\) to \((0, c)\) in the \(x y\)-plane have a constant charge density equal to \(\rho\). Show that the electrostatic potential due to this wire at a point \(\left(x_{1}, y_{1}\right)\) of the \(x y\)-plane is given by $$ \Phi=\rho \log \frac{\sqrt{x_{1}^{2}+\left(c-y_{1}\right)^{2}}+c-y_{1}}{\sqrt{x_{1}^{2}+\left(c+y_{1}\right)^{2}}-c-y_{1}}+k $$ where \(k\) is an arbitrary constant. Show that if \(k\) is chosen so that \(\Phi(1,0)=0\), then, as \(c\) becomes infinite, \(\Phi\) approaches the limiting value \(-2 \rho \log \left|x_{1}\right|\). This is the potential of an infinite wire with uniform charge.

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