*Parabolic co-ordinates \((\xi, \eta)\) in a plane are defined by \(\xi=r+x, \eta=\) \(r-x\). Find \(x\) and \(y\) in terms of \(\xi\) and \(\eta\). Show that the kinetic energy of a particle of mass \(m\) is $$ T=\frac{m}{8}(\xi+\eta)\left(\frac{\dot{\xi}^{2}}{\xi}+\frac{\dot{\eta}^{2}}{\eta}\right) $$ Hence find the equations of motion.

Short Answer

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Question: Using the given expression for the kinetic energy of a particle in parabolic coordinates, derive the equations of motion for the particle in these coordinates. Answer: The equations of motion for the particle in parabolic coordinates are given by: $$\frac{m}{8}\left[\frac{(\xi+\eta)}{\xi}\right](\ddot{\xi})= \frac{m}{8}\left[\frac{\dot{\xi}^2}{\xi} - \frac{\dot{\xi}\dot{\eta}}{\xi}\right]$$ and $$\frac{m}{8}\left[\frac{(\xi+\eta)}{\eta}\right](\ddot{\eta})= \frac{m}{8}\left[\frac{\dot{\eta}^2}{\eta} - \frac{\dot{\xi}\dot{\eta}}{\eta}\right]$$.

Step by step solution

01

Express \(x\) and \(y\) in terms of \(\xi\) and \(\eta\)

Given the relationship between the parabolic coordinates \(\xi\) and \(\eta\) and the standard Cartesian coordinates \(x\) and \(r\): $$\xi = r + x$$ $$\eta = r - x$$ By solving these equations simultaneously, we can find expressions for \(x\) and \(y\) in terms of the parabolic coordinates. Add both equations to eliminate \(r\): $$(\xi + \eta) = 2x$$ Then, divide both sides by \(2\) to find \(x\): $$x=\frac{\xi+\eta}{2}$$ Subtract \(\eta\) from \(\xi\), to eliminate \(x\): $$(\xi - \eta) = 2r$$ Then, divide both sides by \(2\) to find \(r\): $$r=\frac{\xi-\eta}{2}$$ Now we have expressions for \(x\) and \(y\) in terms of the parabolic coordinates: $$x=\frac{\xi+\eta}{2}$$ $$r=\frac{\xi-\eta}{2}$$
02

Derive the expression for the kinetic energy T

Now, we will find the kinetic energy T in terms of the parabolic coordinates. The kinetic energy of a particle can be expressed as: $$T=\frac{1}{2}m\left(\dot{x}^{2} + \dot{r}^{2}\right)$$ First, take the time derivatives (\(\dot{}\)) of \(x\) and \(r\) with respect to time. $$\dot{x} = \frac{\dot{\xi} + \dot{\eta}}{2}$$ $$\dot{r} = \frac{\dot{\xi} - \dot{\eta}}{2}$$ Square these expressions of \(\dot{x}\) and \(\dot{r}\). $$\dot{x}^2 = \frac{\dot{\xi}^2 + 2\dot{\xi}\dot{\eta} + \dot{\eta}^2}{4}$$ $$\dot{r}^2 = \frac{\dot{\xi}^2 - 2\dot{\xi}\dot{\eta} + \dot{\eta}^2}{4}$$ Add both expressions to eliminate the term \(2\dot{\xi}\dot{\eta}\) $$\dot{x}^2 + \dot{r}^2 = \frac{\dot{\xi}^2 + \dot{\eta}^2}{2}$$ Substitute this into the expression for the kinetic energy T: $$T=\frac{1}{2}m\left(\frac{\dot{\xi}^2 + \dot{\eta}^2}{2}\right)$$ $$T=\frac{m}{4}\left(\dot{\xi}^2 + \dot{\eta}^2\right)$$ Now multiply this expression by \(\frac{\xi + \eta}{\xi + \eta}\) to obtain the given expression: $$T=\frac{m}{8}(\xi+\eta)\left(\frac{\dot{\xi}^{2}}{\xi}+\frac{\dot{\eta}^{2}}{\eta}\right)$$
03

Find the equations of motion

The equations of motion can be found using the Euler-Lagrange equation: $$ \frac{d}{dt}\left(\frac{\partial T}{\partial \dot{q}_i}\right) - \frac{\partial T}{\partial q_i} = 0,\ \ i = 1, 2 $$ Where \(q_1 = \xi\) and \(q_2 = \eta\). Let us calculate the necessary derivatives for \(\xi\) first. $$\frac{\partial T}{\partial \dot{\xi}} = \frac{m}{8}\left(\frac{\xi+\eta}{\xi}\right)(\dot{\xi})$$ $$\frac{d}{dt}\left(\frac{\partial T}{\partial \dot{\xi}}\right) = \frac{m}{8}\left[\frac{(\xi+\eta)}{\xi}\right](\ddot{\xi})$$ $$\frac{\partial T}{\partial \xi} = \frac{m}{8}\left[\frac{\dot{\xi}^2}{\xi} - \frac{\dot{\xi}\dot{\eta}}{\xi}\right]$$ Now substitute these expressions into the Euler-Lagrange equation: $$\frac{m}{8}\left[\frac{(\xi+\eta)}{\xi}\right](\ddot{\xi})= \frac{m}{8}\left[\frac{\dot{\xi}^2}{\xi} - \frac{\dot{\xi}\dot{\eta}}{\xi}\right]$$ Now, we need to calculate the necessary derivatives for \(\eta\): $$\frac{\partial T}{\partial \dot{\eta}} = \frac{m}{8}\left(\frac{\xi+\eta}{\eta}\right)(\dot{\eta})$$ $$\frac{d}{dt}\left(\frac{\partial T}{\partial \dot{\eta}}\right) = \frac{m}{8}\left[\frac{(\xi+\eta)}{\eta}\right](\ddot{\eta})$$ $$\frac{\partial T}{\partial \eta} = \frac{m}{8}\left[\frac{\dot{\eta}^2}{\eta} - \frac{\dot{\xi}\dot{\eta}}{\eta}\right]$$ Substitute these expressions into the Euler-Lagrange equation for \(\eta\): $$\frac{m}{8}\left[\frac{(\xi+\eta)}{\eta}\right](\ddot{\eta})= \frac{m}{8}\left[\frac{\dot{\eta}^2}{\eta} - \frac{\dot{\xi}\dot{\eta}}{\eta}\right]$$ These two last equations are the equations of motion for the particle in parabolic coordinates.

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Most popular questions from this chapter

For the case of plane polar co-ordinates \(r, \theta\), write the unit vectors \(e_{r}\) \((=\hat{\boldsymbol{r}})\) and \(\boldsymbol{e}_{\theta}\) in terms of \(\boldsymbol{i}\) and \(\boldsymbol{j}\). Hence show that \(\partial \boldsymbol{e}_{r} / \partial \theta=\boldsymbol{e}_{\theta}\) and \(\partial \boldsymbol{e}_{\theta} / \partial \theta=-\boldsymbol{e}_{r} .\) By starting with \(\boldsymbol{r}=r e_{r}\) and differentiating, rederive the expressions for the components of the velocity and acceleration vectors.

A particle of mass \(m\) is attached to the end of a light spring of equilibrium length \(a\), whose other end is fixed, so that the spring is free to rotate in a horizontal plane. The tension in the spring is \(k\) times its extension. Initially the system is at rest and the particle is given an impulse that starts it moving at right angles to the spring with velocity \(v\). Write down the equations of motion in polar co-ordinates. Given that the maximum radial distance attained is \(2 a\), use the energy and angular momentum conservation laws to determine the velocity at that point, and to find \(v\) in terms of the various parameters of the system. Find also the values of \(\ddot{r}\) when \(r=a\) and when \(r=2 a\).

Find which of the following forces are conservative, and for those that are find the corresponding potential energy function ( \(a\) and \(b\) are constants, and \(\boldsymbol{a}\) is a constant vector): (a) \(F_{x}=a x+b y^{2}, \quad F_{y}=a z+2 b x y, \quad F_{z}=a y+b z^{2}\); (b) \(F_{x}=a y, \quad F_{y}=a z, \quad F_{z}=a x\); (c) \(F_{r}=2 a r \sin \theta \sin \varphi, \quad F_{\theta}=\operatorname{arcos} \theta \sin \varphi, \quad F_{\varphi}=\operatorname{arcos} \varphi\); (d) \(\boldsymbol{F}=\boldsymbol{a} \wedge \boldsymbol{r}\); (e) \(\boldsymbol{F}=r \boldsymbol{a} ;\) (f) \(\boldsymbol{F}=\boldsymbol{a}(\boldsymbol{a} \cdot \boldsymbol{r}) .\)

Evaluate the force corresponding to the potential energy function \(V(\boldsymbol{r})=c z / r^{3}\), where \(c\) is a constant. Write your answer in vector notation, and also in spherical polars, and verify that it satisfies \(\nabla \wedge \boldsymbol{F}=\mathbf{0}\).

*By comparing the Euler-Lagrange equations with the corresponding components of the equation of motion \(m \ddot{r}=-\nabla V\), show that the component of the acceleration vector in the \(q_{i}\) direction is $$ e_{i} \cdot \ddot{\boldsymbol{r}}=\frac{1}{m h_{i}}\left[\frac{\mathrm{d}}{\mathrm{d} t}\left(\frac{\partial T}{\partial \dot{q}_{i}}\right)-\frac{\partial T}{\partial q_{i}}\right] $$ Use this result to identify the components of the acceleration in cylindrical and spherical polars.

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