A particle of mass \(m\) is free to move in a horizontal plane. It is attached to a fixed point \(O\) by a light elastic string, of natural length \(a\) and modulus \(\lambda\). Show that the tension in the string is conservative and show that the Lagrangian for the motion when \(r>a\) is $$ L=\frac{1}{2} m\left(\dot{r}^{2}+r^{2} \dot{\theta}^{2}\right)-\frac{\lambda}{2 a}(r-a)^{2} $$ where \(r\) and \(\theta\) are plane polar coordinates with origin \(O\).

Short Answer

Expert verified
A: The Lagrangian expression for the given system when \(r > a\) is \(L = \frac{1}{2}m(\dot{r}^2 + r^2 \dot{\theta}^2) - \frac{\lambda}{2a}(r - a)^2\).

Step by step solution

01

Tension in the string and its conservativeness

The tension in the elastic string follows Hooke's Law: \(T = \frac{\lambda}{a}(r - a)\), where \(\lambda\) is the modulus and \(a\) is the natural length of the string. We can check if it's conservative by calculating the curl of the force that corresponds to the tension or, equivalently, by checking that it can be derived from a potential energy function. Since we have a radial force, \(\mathbf{F} = T\mathbf{e_r}\), and its curl will be in the \(z\) direction only, we can write: $$ \nabla \times \mathbf{F} = \frac{1}{r} \frac{\partial(T)}{\partial \theta}\mathbf{k} $$ Since tension \(T\) does not depend on \(\theta\), the term \(\frac{\partial(T)}{\partial \theta} = 0\), and thus \(\nabla \times \mathbf{F} = 0\). The tension in the string is conservative.
02

Kinetic energy in plane polar coordinates

In plane polar coordinates, the position vector of the particle is given by \(\mathbf{r} = r\mathbf{e_r}\). The velocity vector can be obtained by taking the time derivative of the position vector: $$ \mathbf{v} = \frac{d \mathbf{r}}{dt} = \dot{r} \mathbf{e_r} + r \dot{\theta} \mathbf{e_\theta} $$ The kinetic energy, \(T\), can be expressed as: $$ T = \frac{1}{2}m\mathbf{v} \cdot \mathbf{v} = \frac{1}{2}m(\dot{r}^2 + r^2 \dot{\theta}^2) $$
03

Potential energy from tension in the string

Since the tension in the string is conservative, there exists a potential energy function, \(V\), such that \(-\nabla V = \mathbf{F}\). Integrating the radial component of the tension force, we obtain the potential energy function as: $$ V(r) = -\int_{a}^{r} T dr' = -\int_{a}^{r} \frac{\lambda}{a}(r' - a) dr' = \frac{\lambda}{2a}(r - a)^2 $$ Note, we have set \(V(a) = 0\) for deriving the above result.
04

Constructing the Lagrangian

The Lagrangian, \(L\), can now be constructed using the expressions for kinetic and potential energy: $$ L = T - V = \frac{1}{2}m(\dot{r}^2 + r^2 \dot{\theta}^2) - \frac{\lambda}{2a}(r - a)^2 $$ This Lagrangian describes the motion of the particle in the plane polar coordinates \((r, \theta)\) for the given system when \(r > a\).

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Most popular questions from this chapter

A system has Lagrangian \(L=\frac{1}{2} T_{a b} v_{a} v_{b}\) where the \(T_{a b} \mathrm{~s}\) are functions of the \(q_{a} \mathrm{~s}\) alone. Show that $$ \frac{\mathrm{d} L}{\mathrm{~d} t}=0 $$ Show that if \(f\) is any function of one variable, then \(L^{\prime}=f(L)\) generates the same dynamics.

\({ }^{\dagger}\) Two particles \(P_{1}\) and \(P_{2}\) have respective masses \(m_{1}\) and \(m_{2}\) and are attracted to each other by a force with time- independent potential \(U(\boldsymbol{r})\), where \(\boldsymbol{r}\) is the vector from \(P_{1}\) to \(P_{2}\). (1) Show that the motion of the centre of mass is the same as in the case \(U=0\). (2) Show that the motion of \(P_{2}\) relative to \(P_{1}\) is the same as in the case that \(P_{1}\) is fixed and \(P_{2}\) is attracted to \(P_{1}\) by a force with potential $$ V=\frac{m_{1}+m_{2}}{m_{1}} U . $$

A particle \(P\) of mass \(m\) is attached to two light inextensible strings, each of length \(a\). The strings pass over two smooth pegs \(A\) and \(B\), which are at the same height and distance \(2 b\) apart. At the other ends of the strings hang two particles of mass \(m\), which can move up and down the vertical lines through \(A\) and \(B\). The particle \(P\) can move in the vertical plane containing \(A\) and \(B\). Show that if \(2 b \cosh \varphi=P A+P B\) and \(2 b \cos \theta=P A-P B\), then the kinetic energy of \(P\) is $$ T=\frac{1}{2} m b^{2}\left(\cosh ^{2} \varphi-\cos ^{2} \theta\right)\left(\dot{\theta}^{2}+\dot{\varphi}^{2}\right) $$ Hence find the Lagrangian of the system in terms of \(\theta\) and \(\varphi\).

A particle of unit mass is moving in the \(x, y\) plane under the influence of the potential $$ U=-\frac{1}{r_{1}}-\frac{1}{r_{2}}, $$ where \(r_{1}\) and \(r_{2}\) are the respective distances from the points \((1,0)\) and \((-1,0)\). Show that if new coordinates are introduced by putting $$ x=\cosh \varphi \cos \theta, \quad y=\sinh \varphi \sin \theta, $$ then the Lagrangian governing the motion becomes $$ L=\frac{1}{2} \Omega\left(\dot{\theta}^{2}+\dot{\varphi}^{2}\right)+2 \Omega^{-1} \cosh \varphi, $$ where \(\Omega=\cosh ^{2} \varphi-\cos ^{2} \theta\). Write down the equations of motion and show that if the particle is set in motion with \(T+U=0\), then $$ \frac{1}{2}\left(\theta^{2}+\dot{\varphi}^{2}\right)-\frac{2 \cosh \varphi}{\Omega^{2}}=0 $$ Deduce that $$ \frac{\mathrm{d}^{2} \theta}{\mathrm{d} \tau^{2}}=0, \quad \frac{\mathrm{d}^{2} \varphi}{\mathrm{d} \tau^{2}}=2 \sinh \varphi $$ where \(\mathrm{d} t / \mathrm{d} \tau=\Omega\). Hence find the path of the particle.

Two particles, each of mass \(m\), are moving under their mutual gravitational attraction, which is given by the potential \(U=-\gamma m / 2 r\), where \(2 r\) is their separation and \(\gamma\) is a constant. Find the equations of motion in terms of the coordinates \(X, Y, Z, r, \theta, \varphi\), where \(X, Y\), and \(Z\) are the Cartesian coordinates of the centre of mass and \(r, \theta\), and \(\varphi\) are the polar coordinates of one particle relative to the centre of mass.

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