/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 83 A uniform, solid cylinder with m... [FREE SOLUTION] | 91Ó°ÊÓ

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A uniform, solid cylinder with mass \(M\) and radius 2\(R\) rests on a horizontal tabletop. A string is attached by a yoke to a frictionless axle through the center of the cylinder so that the cylinder can rotate about the axle. The string runs over a disk-shaped pulley with mass \(M\) and radius \(R\) that is mounted on a frictionless axle through its center. A block of mass \(M\) is suspended from the free end of the string (Fig. 10.62\()\) . The string doesn't slip over the pulley surface, and the cylinder rolls without slipping on the tabletop. Find the magnitude of the acceleration of the block after the system is released from rest.

Short Answer

Expert verified
The acceleration of the block is \(\frac{2}{3}g\).

Step by step solution

01

Analyze the Forces

First, consider the forces acting on the system. For the block of mass \(M\), the gravitational force downward is \(Mg\), where \(g\) is the acceleration due to gravity. For the pulley, the tension \(T\) in the string provides torque. For the solid cylinder rolling on the table, frictional force provides the torque for rolling without slipping.
02

Determine the Torque and Moment of Inertia

For the disk-shaped pulley, the moment of inertia is \(I_\text{pulley} = \frac{1}{2}MR^2\). The torque due to tension is \(\tau = TR\). For the cylinder, which rolls without slipping, the moment of inertia is \(I_\text{cylinder} = \frac{1}{2}M(2R)^2 = 2MR^2\). The frictional force \(f\) does not do work because it acts at the point of contact; however, it ensures no slipping.
03

Apply Newton's Second Law

The equations of motion for the block are given by \(Mg - T = Ma\) where \(a\) is the linear acceleration. For the pulley, the angular acceleration is \(\alpha = \frac{a}{R}\), and Newton's second law for rotation gives us \(TR = \frac{1}{2}MR^2\cdot \alpha\). Substituting \(\alpha\) gives \(TR = \frac{1}{2}MaR\).
04

Connect the Rolling Condition

For the cylinder, the linear acceleration \(a\) is related to the angular acceleration by \(a = R\alpha_\text{cylinder}\). For rolling without slipping, \(f = M'a\), where \(M'\) is the effective mass contribution from the cylinder's rotation, yielding \(f = \frac{1}{2}Ma\).
05

Solve the Equations

Using the equations from Step 3 and friction relation from Step 4, we substitute and solve for \(a\): 1. \(Mg - T = Ma\)2. \(TR = \frac{1}{2}MaR\) gives \(T = \frac{1}{2}Ma\)Substitute \(T\) into the first equation:\(Mg - \frac{1}{2}Ma = Ma\)This simplifies to:\(Mg = \frac{3}{2}Ma\)Solving for \(a\) gives \(a = \frac{2}{3}g\).

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Key Concepts

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

Moment of Inertia
When we talk about rotational dynamics, the idea of moment of inertia frequently comes up. It is essentially the rotational equivalent of mass. Just like mass quantifies an object's resistance to acceleration when a force is applied, the moment of inertia does the same for rotational motion.

In the context of our problem, we need to consider two main components: the disk-shaped pulley and the solid cylinder. The moment of inertia for the disk is given by the formula \(I_\text{pulley} = \frac{1}{2}MR^2\), indicating that the mass is evenly distributed around its center. On the other hand, the moment of inertia for the solid cylinder is \(I_\text{cylinder} = 2MR^2\). This calculation takes into account its geometry and mass distribution, especially since it has a larger radius of \(2R\).

Understanding these values is critical because they influence how easy or difficult it is to set these objects into motion around their respective axes.
Newton's Second Law
Newton's second law is fundamental when analyzing the motion of any object, whether in a straight line or in rotation. This law is summarized as \(F = ma\) for linear motion, where \(F\) is the net force, \(m\) is the mass, and \(a\) is the acceleration.

For the block in our exercise, Newton's second law tells us that the difference between the weight of the block, \(Mg\), and the tension in the string, \(T\), produces its acceleration. We express this as \(Mg - T = Ma\). This is the foundation upon which we balance forces in this interconnected system.

Similarly, in rotational dynamics, Newton's second law is expressed in terms of torque and angular acceleration: \(\tau = I\alpha\). By translating the forces involved in our setup into these rotational terms, we're able to understand how each element of the system moves as a whole.
Rolling Without Slipping
Rolling without slipping is a common and important constraint in physics problems involving wheels and cylinders. It implies that there is no relative motion between the surface of the rolling object and the ground. The point of contact is momentarily at rest, ensuring a clean transfer of rotational motion.

In our exercise, the solid cylinder rolls without slipping on the tabletop. This reveals a relationship between linear and angular quantities. Specifically, the linear acceleration \(a\) of the cylinder's center of mass and its angular acceleration \(\alpha\) satisfy \(a = R\alpha_\text{cylinder}\).

This rolling condition simplifies the problem by providing us an additional equation to relate rotational movement to linear movement, allowing us to solve for unknowns like the acceleration \(a\). The friction at the point of contact, crucially, does not do work but ensures this no-slip condition is maintained.
Torque
Torque can be thought of as the rotational equivalent of force. It measures how effectively a force can produce rotational movement. Torque is given by the product of the force and the distance from the pivot point at which it acts, expressed as \(\tau = F \cdot r\).

In our scenario, the torque plays out in two major ways. For the block-pulley interaction, the tension \(T\) in the string generates torque on the pulley, calculated as \(\tau = TR\). This torque leads to the rotation of the pulley and is subject to its moment of inertia.

The connection of torque and the cylinder involves the frictional force, providing the necessary torque for it to roll. In essence, it's the torque that ensures the energy and momentum are properly distributed throughout the system, linking the linear and rotational equations we use to solve the overall problem.

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Most popular questions from this chapter

A playground merry-go-round has radius 2.40 \(\mathrm{m}\) and moment of inertia 2100 \(\mathrm{kg} \cdot \mathrm{m}^{2}\) about a vertical axle through its center, and it turns with negligible friction. (a) A child applies an 18.0 \(\mathrm{N}\) force tangentially to the edge of the merry-go-round for 15.0 \(\mathrm{s}\) . If the merry-go-round is initially at rest, what is its angular speed after this 15.0 -s interval? (b) How much work did the child do on the merry-go-round? (c) What is the average power supplied by the child?

A stiff uniform wire of mass \(M_{0}\) and length \(L_{0}\) is cut, bent, and the parts soldered together so that it forms a circular wheel having four identical spokes coming out from the center. None of the wire is wasted, and you can neglect the mass of the solder. (a) What is the moment of inertia of this wheel about an axle through its center perpendicular to the plane of the wheel? (b) If the wheel is given an initial spin with angular velocity \(\omega_{0}\) and stops uniformly in time \(T\) , what is the frictional torque at its axle?

Under some circumstances, a star callapse into an extremely dense object made mostly of neurrons and called a neutron star. The density of a neutron star is roughly \(10^{14}\) times as great as that of ordinary solid matter. Suppose we represent the star as a uniform, solid, rigid sphere, both before and after the collapse. The star's initial radius was \(7.0 \times 10^{5} \mathrm{km}\) (comparable to our sun); its final radius is 16 \(\mathrm{km}\) . If the original star rotated once in 30 days, find the angular speed of the neutron star.

A \(55-\mathrm{kg}\) runner runs around the edge of a horizontal turntable mounted on a vertical, frictionless axis through its center. The runner's velocity relative to the earth has magnitude 2.8 \(\mathrm{m} / \mathrm{s}\) . The turntable is rotating in the opposite direction with an angular velocity of magnitude 0.20 \(\mathrm{rad} / \mathrm{s}\) relative to the earth. The radius of the turntable is \(3.0 \mathrm{m},\) and its moment of inertia about the axis of rotation is 80 \(\mathrm{kg} \cdot \mathrm{m}^{2} .\) Find the final angular velocity of the system if the runner comes to rest relative to the turntable. (You can model the runner as a particle.)

A \(2.00-\mathrm{kg}\) textbook rests on a frictionless, horizontal surface. A cord attached to the book passes over a pulley whose diameter is \(0.150 \mathrm{m},\) to a hanging book with mass 3.00 \(\mathrm{kg}\) . The system is released from rest, and the books are observed to move 1.20 \(\mathrm{m}\) in 0.800 \(\mathrm{s}\) s. (a) What is the tension in each part of the cord? \((b)\) What is the moment of inertia of the pulley about its rotation axis?

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