Here are the essential concepts you must grasp in order to answer the question correctly.
Gravitational Force
Gravitational force is the attractive force between two masses, described by Newton's law of universal gravitation. It states that the force is proportional to the product of the two masses and inversely proportional to the square of the distance between their centers. In this scenario, the gravitational force exerted by the rod on the sphere must be calculated by integrating the contributions from each infinitesimal mass element of the rod.
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Potential Energy (U)
Potential energy in the context of gravitational interactions is the energy stored due to the position of an object in a gravitational field. It can be expressed as U = -G(m1*m2)/r, where G is the gravitational constant, m1 and m2 are the masses, and r is the distance between them. The change in potential energy with respect to position is crucial for determining the force acting on the sphere, as the gravitational force can be derived from the negative gradient of the potential energy.
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Differentiation and Force Calculation
The relationship between force and potential energy is given by the equation Fx = -dU/dx, which states that the force is the negative derivative of potential energy with respect to position. This means that to find the gravitational force acting on the sphere, one must differentiate the potential energy function with respect to the distance x. This approach allows for the calculation of the force at any position, including the limit where x is much larger than L, simplifying the analysis.
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