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Ch 15: Oscillations
Chapter 15, Problem 13

FIGURE CP13.71 shows a particle of mass m at distance 𝓍 from the center of a very thin cylinder of mass M and length L. The particle is outside the cylinder, so 𝓍 > L/2 . (a) Calculate the gravitational potential energy of these two masses.

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Identify the formula for gravitational potential energy between two point masses, which is given by U = -G \frac{m_1 m_2}{r}, where G is the gravitational constant, m_1 and m_2 are the masses, and r is the distance between the centers of the two masses.
Recognize that the cylinder can be approximated as a line of mass, and the problem can be approached by integrating the contributions to the gravitational potential energy from each infinitesimal mass element dm along the length of the cylinder.
Set up the integral for the gravitational potential energy. Let dm = \frac{M}{L} dx, where M is the total mass of the cylinder and L is its length. The variable x will vary from -L/2 to L/2 along the cylinder.
Express the distance from the particle to an element dm of the cylinder as a function of x. Since the particle is at a distance x_0 from the center of the cylinder, the distance to a point at x along the cylinder is r = \sqrt{x_0^2 + x^2}.
Integrate the expression for the potential energy U = -G \int_{-L/2}^{L/2} \frac{m dm}{r} = -Gm \int_{-L/2}^{L/2} \frac{M/L}{\sqrt{x_0^2 + x^2}} dx, where x_0 is the distance from the center of the cylinder to the particle. This integral will give the total gravitational potential energy between the particle and the cylinder.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Gravitational Potential Energy

Gravitational potential energy (U) is the energy an object possesses due to its position in a gravitational field. It is calculated using the formula U = -G(m1*m2)/r, where G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between their centers of mass. This concept is crucial for understanding how mass interacts with gravity and how energy is stored in gravitational fields.
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Newton's Law of Universal Gravitation

Newton's Law of Universal Gravitation states that every point mass attracts every other point mass in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. This law provides the foundation for calculating gravitational forces and potential energy in systems involving multiple masses, such as the particle and cylinder in the question.
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Distance in Gravitational Calculations

In gravitational calculations, the distance between the centers of mass of the interacting bodies is critical. For a particle outside a cylinder, the effective distance used in potential energy calculations must account for the geometry of the system. Understanding how to determine this distance, especially when the particle is outside the cylinder, is essential for accurately calculating the gravitational potential energy.
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Related Practice
Textbook Question
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Textbook Question
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