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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 \(\varphi\).

Short Answer

Expert verified
Answer: The Lagrangian of the system is given by \(L = \frac{1}{2} m b^2 \left(\cosh^2\varphi - \cos^2\theta\right)\left(\dot{\theta}^2 + \dot{\varphi}^2\right)\), where m is the mass of the particle and b is a geometric variable that depends on the lengths of the strings.

Step by step solution

01

Relationship of PA and PB with θ and φ

First, let's express lengths PA and PB in terms of angle variables, θ and φ. Consider triangle AOP (where O is the midpoint of AB) and use the Law of Cosines: $$ PA^2 = a^2 + b^2 - 2ab\cos \theta$$ Now, consider triangle BOP and apply Law of Cosines: $$ PB^2 = a^2 + b^2 + 2ab\cos \theta$$ Adding both equations yields: $$ PA^2 + PB^2 = 2a^2 + 4b^2 \Rightarrow 2b\cosh\varphi = PA + PB$$ Subtracting second equation from the first one results in: $$ PA^2 - PB^2 = -4ab\cos\theta \Rightarrow 2b\cos\theta = PA - PB$$
02

Finding the velocities of P with respect to θ and φ

Differentiate the expressions for PA and PB with respect to time to get the velocities: $$\dot{PA} = \frac{-2ab\sin\theta}{2b\cos\theta} \dot{\theta} = -\tan\theta\dot{\theta}$$ $$\dot{PB} = \frac{2ab\sin\theta}{2b\cos\theta} \dot{\theta} = \tan\theta\dot{\theta}$$
03

Finding the kinetic energy

Now we can express the kinetic energy in terms of the given variables: $$ T = \frac{1}{2} m \left(\dot{PA}^2 + \dot{PB}^2\right) = \frac{1}{2} m \left(\tan^2\theta\dot{\theta}^2 + \tan^2\theta\dot{\theta}^2\right)$$ Substitute the expression for \(\tan\theta\) from step 1: $$ T = \frac{1}{2} m b^2 \left(\cosh^2\varphi - \cos^2\theta\right)\left(\dot{\theta}^2 + \dot{\varphi}^2\right)$$
04

Finding the Lagrangian

To find the Lagrangian (\(L\)) of the system in terms of θ and φ, we need to express the kinetic energy in terms of the generalized coordinates. Since there are no external forces acting on the system, the potential energy will remain constant. Therefore, the Lagrangian of the system is equal to the kinetic energy (\(T\)): $$ L = T = \frac{1}{2} m b^2 \left(\cosh^2\varphi - \cos^2\theta\right)\left(\dot{\theta}^2 + \dot{\varphi}^2\right) $$ This expression represents the Lagrangian of the system in terms of the angles \(\theta\) and \(\varphi\).

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Most popular questions from this chapter

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.

\({ }^{\dagger}\) 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 of unit mass is subject to an inverse-square-law central force $$ \boldsymbol{F}=-\frac{\boldsymbol{r}}{r^{3}} $$ where \(r=|\boldsymbol{r}|\) and \(\boldsymbol{r}\) is the position vector from the origin of an inertial frame. Show that the motion is governed by the Lagrangian $$ L=\frac{1}{2} \dot{r} \cdot \dot{r}+\frac{1}{r} $$ Write down the equations of motion in spherical polar coordinates and show that there are solutions with \(\theta=\pi / 2\) throughout the motion.

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A particle of mass \(m\) is constrained to move under gravity on the surface of a smooth right circular cone of semi-vertical angle \(\pi / 4\). The axis of the cone is vertical, with the vertex downwards. Find the equations of motion in terms of \(z\) (the height above the vertex) and \(\theta\) (the angular coordinate around the circular cross-sections). Show that $$ \dot{z}^{2}+\frac{h^{2}}{2 z^{2}}+g z=E $$ where \(E\) and \(h\) are constant. Sketch and interpret the trajectories in the \(z, \dot{z}\)-plane for a fixed value of \(h\).

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