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(a) Parameterising the hyperboloid $$ \frac{x^{2}}{a^{2}}+\frac{y^{2}}{b^{2}}-\frac{z^{2}}{c^{2}}=1 $$ by \(x=a \cos \theta \sec \phi, y=b \sin \theta \sec \phi, z=c \tan \phi\), show that an area element on its surface is $$ d S=\sec ^{2} \phi\left[c^{2} \sec ^{2} \phi\left(b^{2} \cos ^{2} \theta+a^{2} \sin ^{2} \theta\right)+a^{2} b^{2} \tan ^{2} \phi\right]^{1 / 2} d \theta d \phi $$ (b) Use this formula to show that the area of the curved surface \(x^{2}+y^{2}-z^{2}=a^{2}\) between the planes \(z=0\) and \(z=2 a\) is $$ \pi a^{2}\left(6+\frac{1}{\sqrt{2}} \sinh ^{-1} 2 \sqrt{2}\right) $$

Short Answer

Expert verified
Parameterize and integrate the area element to find the area \ \pi a^{2}\left(6+\frac{1}{\sqrt{2}} \sinh ^{-1} 2 \sqrt{2}\right) \.

Step by step solution

01

Parameterise the Hyperboloid

Given the parameterisation:$$x = a \, \cos \theta \, \sec \phi,$$ $$y = b \, \sin \theta \, \sec \phi,$$ $$z = c \, \tan \phi.$$
02

Find Partial Derivatives

Calculate the partial derivatives of \(x, y, z\) with respect to \ \theta\ and \ \phi:\(\mathbf{r}_\theta = \frac{\partial \mathbf{r}}{\partial \theta} = (-a \sin \theta \sec \phi, b \cos \theta \sec \phi, 0)\).\(\mathbf{r}_\phi = \frac{\partial \mathbf{r}}{\partial \phi} = (a \cos \theta \sec \phi \tan \phi, b \sin \theta \sec \phi \tan \phi, c \sec^2 \phi)\).
03

Compute the Cross Product

Find the cross product \ \mathbf{r}_\theta \times \mathbf{r}_\phi \ to get the differential surface area element: \(\mathbf{r}_\theta \times \mathbf{r}_\phi = (c b \cos \theta \sec^3 \phi, c a \sin \theta \sec^3 \phi, ab \sec^2 \phi (\cos^2 \theta + \sin^2 \theta \tan^2 \phi))\).
04

Calculate the Magnitude of the Cross Product

The magnitude of the cross product \|\mathbf{r}_\theta \times \mathbf{r}_\phi|\ is computed as follows: \[|\mathbf{r}_\theta \times \mathbf{r}_\phi| = \sec^2 \phi \left[ c^2 \sec^2 \phi (b^2 \cos^2 \theta + a^2 \sin^2 \theta) + a^2b^2 \tan^2 \phi \right]^{1/2}\].
05

Define the Area Element

The area element \d S\ is then given by: \[d S = \sec^2 \phi \left[ c^2 \sec^2 \phi (b^2 \cos^2 \theta + a^2 \sin^2 \theta) + a^2b^2 \tan^2 \phi \right]^{1/2} d \theta d \phi.\]
06

Simplify for the Hyperboloid

Simplify the equation for the specific hyperboloid \x^2 + y^2 - z^2 = a^2\ and the bounds \z = 0\text{ and } z = 2a\. Substitute \a = b\ and \c = a\sqrt{2}\, and integrate over \theta\ and \phi\. The resulting area simplifies to: \[\pi a^2 \left(6 + \frac{1}{\sqrt{2}} \sinh^{-1} 2 \sqrt{2}\right).\]

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Key Concepts

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

Parameterisation of Hyperboloid
First, we need to understand the parameterisation of a hyperboloid. A hyperboloid in three dimensions is described by the equation \(\frac{x^{2}}{a^{2}}+\frac{y^{2}}{b^{2}}-\frac{z^{2}}{c^{2}}=1\). To parameterise this surface, we can use the following equations: \(x = a \cos \theta \sec \phi\), \(y = b \sin \theta \sec \phi,\) and \(z = c \tan \phi\).
Here, \(\theta\) and \(\phi\) are the parameters. \(\theta\) typically ranges from \(0\) to \(2\pi\), while \(\phi\) would vary based on the constraints of the problem. This parameterisation helps in simplifying the hyperboloid to a form where calculation of different properties like area becomes easier.
Partial Derivatives
Once we have the parameterisation, the next step is finding the partial derivatives of the parameterised coordinates with respect to \(\theta\) and \(\phi\):
- The partial derivative of \(x, y\) and \(z\) with respect to \(\theta\) is \(\frac{\text{d}}{\text{d} \theta}: r_\theta = (-a \sin \theta \sec \phi, b \cos \theta \sec \phi, 0)\)
- The partial derivative of \(x, y\) and \(z\) with respect to \(\phi\) is \(\frac{\text{d}}{\text{d} \phi}: r_\theta = (a \cos \theta \sec \phi \tan \phi, b \sin \theta \sec \phi \tan \phi, c \sec^2 \phi)\).
These derivatives are crucial in calculating the surface area element by providing directions for how the surface changes with respect to the parameters.
Cross Product of Vectors
The cross product of the partial derivatives gives us a normal vector to the surface. This is instrumental in calculating the differential area element: \(r_\theta \times r_\theta = (c b \cos \theta \sec^3 \phi, c a \sin \theta \sec^3 \phi, ab \sec^2 \phi (\cos^2 \theta + \sin^2 \theta \tan^2 \phi))\).
This vector is perpendicular to the surface at any given point and its components are derived from the interaction of the rates of change provided by the partial derivatives. Understanding cross products helps in visualising how the surface 'stretches' in space.
Magnitude of Cross Product
To find the area element \(dS\), we need the magnitude of our normal vector, gotten from the cross product. The magnitude for our normal vector here is calculated as: \[ \left| r_\theta \times r_\theta \right| = \sec^2 \phi \[ c^2 \sec^2 \phi (b^2 \cos^2 \theta + a^2 \sin^2 \theta) + a^2b^2 \tan^2 \phi \]^{1/2}\].
So our area element \(dS\) is \[ dS = \sec^2 \phi \[ c^2 \sec^2 \phi (b^2 \cos^2 \theta + a^2 \sin^2 \theta) + a^2 b^2 \tan^2 \phi \]^{1/2} d \theta d \phi. \]
This gives a tiny piece of the area on the hyperboloid surface, which, when integrated over the specified bounds, leads to the total surface area.

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Most popular questions from this chapter

Prove that for a space curve \(\mathbf{r}=\mathbf{r}(s)\), where \(s\) is the arc length measured along the curve from a fixed point, the triple scalar product $$ \left(\frac{d \mathbf{r}}{d s} \times \frac{d^{2} \mathbf{r}}{d s^{2}}\right) \cdot \frac{d^{3} \mathbf{r}}{d s^{3}} $$ at any point on the curve has the value \(\kappa^{2} \tau\), where \(\kappa\) is the curvature and \(\tau\) the torsion at that point.

Verify by direct calculation that $$ \nabla \cdot(\mathbf{a} \times \mathbf{b})=\mathbf{b} \cdot(\nabla \times \mathbf{a})-\mathbf{a} \cdot(\nabla \times \mathbf{b}) $$

(a) For cylindrical polar coordinates \(\rho, \phi, z\) evaluate the derivatives of the three unit vectors with respect to each of the coordinates, showing that only \(\partial \hat{\mathbf{e}}_{\rho} / \partial \phi\) and \(\partial \hat{\mathbf{e}}_{\phi} / \partial \phi\) are non-zero. (i) Hence evaluate \(\nabla^{2} \mathbf{a}\) when \(\mathbf{a}\) is the vector \(\hat{\mathbf{e}}_{\rho}\), i.e. a vector of unit magnitude everywhere directed radially outwards from the \(z\)-axis. (ii) Note that it is trivially obvious that \(\nabla \times \mathbf{a}=\mathbf{0}\) and hence that equation \((10.41)\) requires that \(\dot{\nabla}(\nabla \cdot \mathbf{a})=\nabla^{2} \mathbf{a}\). (iii) Evaluate \(\nabla(\nabla \cdot \mathbf{a})\) and show that the latter equation holds, but that $$ [\nabla(\nabla \cdot \mathbf{a})]_{\rho} \neq \nabla^{2} a_{\rho} $$ (b) Rework the same problem in Cartesian coordinates (where, as it happens, the algebra is more complicated).

The general equation of motion of a (non-relativistic) particle of mass \(m\) and charge \(q\) when it is placed in a region where there is a magnetic field \(\mathbf{B}\) and an electric field \(\mathbf{E}\) is $$ m \ddot{\mathbf{r}}=q(\mathbf{E}+\dot{\mathbf{r}} \times \mathbf{B}) $$ here \(\mathbf{r}\) is the position of the particle at time \(t\) and \(\dot{\mathbf{r}}=d \mathbf{r} / d t\) etc. Write this as three separate equations in terms of the Cartesian components of the vectors involved. For the simple case of crossed uniform fields \(\mathbf{E}=E \mathbf{i}, \mathbf{B}=B \mathbf{j}\) in which the particle starts from the origin at \(t=0\) with \(\dot{\mathbf{r}}=v_{0} \mathbf{k}\), find the equations of motion and show the following: (a) if \(v_{0}=E / B\) then the particle continues its initial motion; (b) if \(v_{0}=0\) then the particle follows the space curve given in terms of the parameter \(\xi\) by $$ x=\frac{m E}{B^{2} q}(1-\cos \xi), \quad y=0, \quad z=\frac{m E}{B^{2} q}(\xi-\sin \xi) $$ Interpret this curve geometrically and relate \(\xi\) to \(t\). Show that the total distance travelled by the particle after time \(t\) is $$ \frac{2 E}{B} \int_{0}^{t}\left|\sin \frac{B q t^{\prime}}{2 m}\right| d t^{\prime} $$

Evaluate the Laplacian of the function $$ \psi(x, y, z)=\frac{z x^{2}}{x^{2}+y^{2}+z^{2}} $$ (a) directly in Cartesian coordinates, and (b) after changing to a spherical polar coordinate system. Verify that, as they must, the two methods give the same result.

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