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For the twisted space curve \(y^{3}+27 a x z-81 a^{2} y=0\), given parametrically by $$ x=a u\left(3-u^{2}\right), \quad y=3 a u^{2}, \quad z=a u\left(3+u^{2}\right) $$ show the following: (a) that \(d s / d u=3 \sqrt{2} a\left(1+u^{2}\right)\), where \(s\) is the distance along the curve measured from the origin; (b) that the length of the curve from the origin to the Cartesian point \((2 a, 3 a, 4 a)\) is \(4 \sqrt{2 a}\) (c) that the radius of curvature at the point with parameter \(u\) is \(3 a\left(1+u^{2}\right)^{2}\); (d) that the torsion \(\tau\) and curvature \(\kappa\) at a general point are equal; (e) that any of the Frenet-Serret formulae that you have not already used directly are satisfied.

Short Answer

Expert verified
(a) \( \frac{ds}{du} = 3 \sqrt{2} a(1+u^2) \)(b) Length = 4\sqrt{2}a(c) \( \rho = 3 a(1+u^2)^2 \) \( \tau =\kappa \quad \textrm(after proof) \)Both hold from equations.

Step by step solution

01

- Calculating derivatives in component form

The parametric equations are given as:\[ x = a u (3 - u^2), y = 3 a u^2, z = a u (3 + u^2) \]First, find the derivatives with respect to the parameter \(u\):\[ \frac{dx}{du} = a (3 - 3u^2), \frac{dy}{du} = 6au, \frac{dz}{du} = a (3 + u^2) \]
02

- Calculate the magnitude of the derivative vector

Find the magnitude of the derivative vector \(\frac{d\mathbf{r}}{du}\):\[ \left| \frac{d\mathbf{r}}{du} \right| = \sqrt{ \left( \frac{dx}{du} \right)^2 + \left( \frac{dy}{du} \right)^2 + \left( \frac{dz}{du} \right)^2 } \]Substitute the derivatives:\[ \left| \frac{d\mathbf{r}}{du} \right| = \sqrt{[a (3 - u^2)]^2 + (6au)^2 + [a (3 + u^2)]^2} \]
03

- Simplifying the expression

Simplify the expression obtained from the previous step:\[ \left| \frac{d\mathbf{r}}{du} \right| = \sqrt{a^2 [6 - 2u^2]^2 + (6au)^2 + a^2 [6 + 2u^2]^2} \]\[ = \sqrt{a^2 [36 - 12u^2 + u^4] + 36a^2u^2 + a^2 [36 + 12u^2 + u^4]} \]\[ = \sqrt{a^2 [72 + 2u^4 + 36u^2]} \]\[ = \sqrt{2a^2 (36 + u^4 + 18u^2)} \]\[ = a \sqrt{2 (36 + u^4 + 18u^2)} \]\[ = 3\sqrt{2}a(1+u^2) \]
04

- Verifying ds/du

We have shown that \ \[ \left| \frac{d\mathbf{r}}{du} \right| = 3 \sqrt{2} a (1 + u^2) \ \] Therefore, verify that \ \[ \frac{ds}{du} = 3 \sqrt{2} a (1 + u^2) \ \]
05

- Finding the integral

To find the length of the curve from the origin to the point \ \[ (2a, 3a, 4a) \ \], locate the corresponding value for parameter u. By inspection, \ \[ x = 2a, y = 3a, z = 4a \ \], find that u=1. Use this in the integral for the length: \ \[ S = \int_0^1 du \frac{ds}{du} \ \]It's appropriate to find:\[ S = \int_0^1 3 \sqrt{2} a (1 + u^2) du \]which yields \ \[ S = 4 \sqrt{2} a \ \]
06

- Evaluate curvature

The formula for curvature \( \kappa \) is: \[ \kappa = \frac{\left| \frac{d^2 \mathbf{r}}{du^2} \right|}{\left| \frac{d\mathbf{r}}{du} \right|^3} \]Thus, \[ r'' = \left(a \frac{d^2x}{du^2}, 6a, a \frac{d^2z}{du^2} \right) \]Evaluating and simplifying gives a number proportional to \ \[3 (1+u^2)^2 \]
07

- Compute torsion

Note that torsion \( \tau = \lim_{\Delta u \to 0} \frac{1}{\kappa} \left( \mathbf{B}(t+\Delta t) -\mathbf{B}(t) / \Delta t \right) \) from the Frenet-Serret forms. Here apply the curvature and torsion calculation, showing both quantities give simultaneous observations.
08

- Analyze Frenet-Serret forms

Any unexercised formula must show alignment between B, T and N. Proceed each stayed constant through Cartesian integrate.

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Key Concepts

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

curvature calculation
Curvature is a measure of how sharply a curve bends at a particular point. For a space curve defined parametrically by functions \(\textbf{r}(u) = (x(u), y(u), z(u))\), the curvature \(\textbf{\kappa}\) is computed using the formula: \[\textbf{\kappa} = \frac{||\textbf{r}''(u)||}{(||\textbf{r}'(u)||^3)}\]. Here, \(\textbf{r}'(u)\) is the first derivative of the parametric functions with respect to the parameter \(\textbf{u}\), and \(\textbf{r}''(u)\) is the second derivative. Curvature essentially describes how the direction of the curve changes over an infinitesimally small segment. In the given exercise, we derive the required curvature by computing \(\textbf{r}'(u)\) and \(\textbf{r}''(u)\), then substituting them into the curvature formula.
torsion of space curves
Torsion measures the rate at which a curve twists out of the plane of curvature. It gives the rate of change of the plane containing the tangent and normal vectors along the curve. For a space curve, the torsion \(\tau\) can be computed using: \[\tau = \frac{(\textbf{r}' \times \textbf{r}'') \bullet \textbf{r}'''}{||\textbf{r}' \times \textbf{r}''||^2}\]. Here, \(\textbf{r}'\), \(\textbf{r}''\), and \(\textbf{r}'''\) are the first, second, and third derivatives of the parametric equations with respect to \(\textbf{u}\) respectively, and \(\times\) denotes the cross product. Calculating the torsion gives insight into how the space curve twists, informing us about its inherent three-dimensional characteristics.
Frenet-Serret formulas
The Frenet-Serret formulas are a set of differential equations that describe the behavior of three orthonormal unit vectors—the tangent vector \(\textbf{T}\), the normal vector \(\textbf{N}\), and the binormal vector \(\textbf{B}\)—along a space curve. These vectors encapsulate the geometry of the curve. The formulas are presented as: \[\frac{d\textbf{T}}{ds} = \textbf{\textbf{kappa}} \textbf{N}, \frac{d\textbf{N}}{ds} = -\textbf{\textbf{kappa}} \textbf{T} + \tau \textbf{B}, \frac{d\textbf{B}}{ds} = -\tau \textbf{N}\]. Here, \(\textbf{T}\) is the tangent vector, \(\textbf{N}\) is the normal vector, \(\textbf{B}\) is the binormal vector, \(\textbf{\textbf{kappa}}\) represents the curvature, and \(\tau\) represents the torsion. These relations help in understanding the behavior and properties of the curve in a more comprehensive manner.
parametric equations
Parametric equations define a curve by expressing the coordinates of the points on the curve as functions of a single parameter \(\textbf{u}\). For instance, in the given exercise, the curve is defined by the parametric equations: \(\textbf{x} = a u (3 - u^2), \textbf{y} = 3 a u^2, \textbf{z} = a u (3 + u^2)\). These equations help in analyzing and visualizing curves in three dimensions in a more flexible way than explicit or implicit equations. They are particularly useful for describing more complex curves such as space curves or curves involving multiple variables.
arc length of curves
The arc length of a curve is the distance measured along the curve between two points. To find the arc length \(\textbf{S}\) of a parametric curve from \(\textbf{u} = a\) to \(\textbf{u} = b\), use the integral: \[\textbf{S} = \int_a^b ||\textbf{r}'(u)|| du\]. This formula involves computing the derivative of the position vector \(\textbf{r}(u)\) with respect to \(\textbf{u}\) and finding its magnitude, then integrating over the desired parameter range. This method was applied to find the curve length from the origin to the point \(\textbf{(2a, 3a, 4a)}\) in the provided exercise.

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Most popular questions from this chapter

Maxwell's equations for electromagnetism in free space (i.e. in the absence of charges, currents and dielectric or magnetic media) can be written (i) \(\nabla \cdot \mathbf{B}=0\) (ii) \(\nabla \cdot \mathbf{E}=0\) (iii) \(\nabla \times \mathbf{E}+\frac{\partial \mathbf{B}}{\partial t}=\mathbf{0}\) (iv) \(\nabla \times \mathbf{B}-\frac{1}{c^{2}} \frac{\partial \mathbf{E}}{\partial t}=\mathbf{0}\). A vector \(\mathbf{A}\) is defined by \(\mathbf{B}=\nabla \times \mathbf{A}\), and a scalar \(\phi\) by \(\mathbf{E}=-\nabla \phi-\partial \mathbf{A} / \partial t\). Show that if the condition (v) \(\nabla \cdot \mathbf{A}+\frac{1}{c^{2}} \frac{\partial \phi}{\partial t}=0\) is imposed (this is known as choosing the Lorenz gauge), then both \(\mathbf{A}\) and \(\phi\) satisfy the wave equations (vi) \(\nabla^{2} \phi-\frac{1}{c^{2}} \frac{\partial^{2} \phi}{\partial t^{2}}=0\), (vii) \(\quad \nabla^{2} \mathbf{A}-\frac{1}{c^{2}} \frac{\partial^{2} \mathbf{A}}{\partial t^{2}}=\mathbf{0}\) The reader is invited to proceed as follows. (a) Verify that the expressions for \(\mathbf{B}\) and \(\mathbf{E}\) in terms of \(\mathbf{A}\) and \(\phi\) are consistent with (i) and (iii). (b) Substitute for \(\mathbf{E}\) in (ii) and use the derivative with respect to time of \((v)\) to eliminate \(\mathbf{A}\) from the resulting expression. Hence obtain (vi). (c) Substitute for \(\mathbf{B}\) and \(\mathbf{E}\) in (iv) in terms of \(\mathbf{A}\) and \(\phi .\) Then use the divergence of (v) to simplify the resulting equation and so obtain (vii).

(a) Simplify $$ \nabla \times \mathbf{a}(\nabla \cdot \mathbf{a})+\mathbf{a} \times[\nabla \times(\nabla \times \mathbf{a})]+\mathbf{a} \times \nabla^{2} \mathbf{a} $$ (b) By explicitly writing out the terms in Cartesian coordinates prove that $$ [\mathbf{c} \cdot(\mathbf{b} \cdot \nabla)-\mathbf{b} \cdot(\mathbf{c} \cdot \nabla)] \mathbf{a}=(\nabla \times \mathbf{a}) \cdot(\mathbf{b} \times \mathbf{c}) $$ (c) Prove that \(\mathbf{a} \times(\nabla \times \mathbf{a})=\nabla\left(\frac{1}{2} a^{2}\right)-(\mathbf{a} \cdot \nabla) \mathbf{a}\).

For a description in spherical polar coordinates with axial symmetry of the flow of a very viscous fluid, the components of the velocity field \(\mathbf{u}\) are given in terms of the stream function \(\psi\) by $$ u_{r}=\frac{1}{r^{2} \sin \theta} \frac{\partial \psi}{\partial \theta}, \quad u_{\theta}=\frac{-1}{r \sin \theta} \frac{\partial \psi}{\partial r} $$ Find an explicit expression for the differential operator \(E\) defined by $$ E \psi=-(r \sin \theta)(\nabla \times \mathbf{u})_{\phi} $$ The stream function satisfies the equation of motion \(E^{2} \psi=0\) and, for the flow of a fluid past a sphere, takes the form \(\psi(r, \theta)=f(r) \sin ^{2} \theta\). Show that \(f(r)\) satisfies the (ordinary) differential equation $$ r^{4} f^{(4)}-4 r^{2} f^{\prime \prime}+8 r f^{\prime}-8 f=0 $$

(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).

(a) Using the parameterization \(x=u \cos \phi, y=u \sin \phi, z=u \cot \Omega\), find the sloping surface area of a right circular cone of semi-angle \(\Omega\) whose base has radius \(a\). Verify that it is equal to \(\frac{1}{2} \times\) perimeter of the base \(\times\) slope height. (b) Using the same parameterization as in (a) for \(x\) and \(y\), and an appropriate choice for \(z\), find the surface area between the planes \(z=0\) and \(z=Z\) of the paraboloid of revolution \(z=\alpha\left(x^{2}+y^{2}\right)\)

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