Chapter 17: Problem 27
27\. Find the cone of least surface area with given volume \(V\) (Simpson).
Short Answer
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Chapter 17: Problem 27
27\. Find the cone of least surface area with given volume \(V\) (Simpson).
These are the key concepts you need to understand to accurately answer the question.
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Get started for free36\. Replace \(x\) by \(i x\) in the expansion in the text for \(\left(e^{x}-\right.\) \(\left.e^{-x}\right) / 2\) to get both the power series for the sine and a representation of the sine as an infinite product. By using the relationship between the roots and coefficients of a polynomial (extended to power series), show that $$ \sum_{k=1}^{\infty} \frac{1}{k^{2}}=\frac{\pi^{2}}{6} \text { and } \sum_{k=1}^{\infty} \frac{1}{k^{4}}=\frac{\pi^{4}}{90} $$
Show that the equation \(a \pm c x / b=\sqrt{x^{2}+y^{2}}\) is a parabola if
\(b=c\), is an ellipse if \(b>c\), and is a hyperbola if \(b
24\. Suppose that the solution to the wave equation \(\frac{2^{2} y}{\partial t^{2}}=\frac{\partial^{2} y}{\partial x^{2}}\) is given by \(y=\Psi(t+x)-\Psi(t-x)\). Show that the initial conditions \(y(0, x)=f(x), y^{\prime}(0, x)=g(x)\) and the condition \(y(t, 0)=y(t, l)=0\) for all \(t\) lead to the requirements that \(f(x)\) and \(g(x)\) are odd functions of period \(2 l\) (d'Alembert).
The modern way to derive Kepler's area law is to break the force into its radial and transverse components, rather than the tangential and normal components used by Hermann, and use polar coordinates whose origin is the center of force. Assume then that the center of force is at the origin of a polar coordinate system. Using vector notation, \(\operatorname{set} \mathbf{u}_{r}=\mathbf{i} \cos \theta+\mathbf{j} \sin \theta\) and \(\mathbf{u}_{\theta}=-\mathbf{i} \sin \theta+j \cos \theta .\) Show that \(d \mathbf{u}_{r} / d \theta=\mathbf{u}_{\theta}\) and \(d \mathbf{u}_{\theta} / d \theta=-\mathbf{u}_{r}\). Then show that if \(\mathbf{r}=r \mathbf{u}_{r}\), then the velocity \(\mathbf{v}\) is given by \(r(d \theta / d t) \mathbf{u}_{\theta}+\) \((d r / d t) \mathbf{u}_{r}\). Show next that the radial component \(a_{r}\) and the transverse component \(a_{\theta}\) of the acceleration are given by $$ a_{r}=\frac{d^{2} r}{d t^{2}}-r\left(\frac{d \theta}{d t}\right)^{2} \quad \text { and } \quad a_{\theta}=r \frac{d^{2} \theta}{d t^{2}}+2 \frac{d r}{d t} \frac{d \theta}{d t} $$ Since the force is central, \(a_{\theta}=0 .\) Multiply the differential equation expressing that fact by \(r\) and integrate to get \(r^{2} \frac{d \theta}{d t}=k\), where \(k\) is a constant. Show finally that \(r^{2} \frac{d \theta}{d t}=\) \(\frac{d A}{d t}\), where \(A\) is the area swept out by the radius vector. This proves Kepler's law of areas.
Translate Leibniz's solution of \(m d x+n y d x+d y=0\) into modern terms by noting that \(d p / p=n d x\) is equiv-
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