Potential energy increase of an expanding stellar object

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The discussion centers on calculating the energy required to double the radius of a uniformly dense stellar object, expressed in terms of mass and radius. Participants emphasize the importance of demonstrating an effort to solve the problem before seeking help. A link to homework guidelines is provided, highlighting the need for adherence to forum rules. The thread is ultimately closed, indicating that no further responses will be given until the original poster follows the proper procedure. Engaging with the community requires an initial attempt at problem-solving.
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How much energy is required to double the radius of a uniformly dense stellar object? Express the answer in terms of mass and the radius of the object.
 
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Please repost in the homework forum with an attempt at a solution.

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I built a device designed to brake angular velocity which seems to work based on below, i used a flexible shaft that could bow up and down so i could visually see what was happening for the prototypes. If you spin two wheels in opposite directions each with a magnitude of angular momentum L on a rigid shaft (equal magnitude opposite directions), then rotate the shaft at 90 degrees to the momentum vectors at constant angular velocity omega, then the resulting torques oppose each other...

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