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Question #42388
The Question
A spherical dust cloud of mass and radius initially has a uniform density and rotates with an angular velocity . It undergoes gravitational collapse, radiating away energy, until it settles into a new spherical shape of radius . In this final state, the cloud has a non-uniform density profile given by (where is a constant and is the distance from the center). Assuming no external torques act on the system, what is the net energy radiated away during this process?
Options
- A.
- B.
- C.
- D.
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Correct Answer
Step-by-Step Solution
Explanation
How the Examiner Thinks
Multi-Concept_Bridge
Master problems that require linking physics and math concepts to solve complex competitive questions.
Concepts Behind This Question
Work-Energy Theorem for Rotation|Gravitational Self-Energy|Integration
Why This Question Is Tricky
Common Mistakes
This question tests the interplay between the Work-Energy Theorem, Gravitational Self-Energy, and Angular Momentum conservation during mass redistribution.
The primary trap is assuming the moment of inertia scales simply as without accounting for the non-uniform density profile , which alters both the final moment of inertia and the gravitational self-energy.
Students often incorrectly apply the uniform sphere formulas and to the final state, failing to integrate over the new mass distribution.
This forces the realization that rotational kinetic energy gain is explicitly balanced by the change in internal gravitational potential energy.
Quick Facts About This Question
Question Information
| Subject | Physics |
| Chapter | System of Particles and Rotational Motion - Class 11 Part 1 |
| Concept | Work-Energy Theorem for Rotation |
| Difficulty | 8 |
| Cognitive Load | 7 |
| Target Solve Time | 160 sec |
| Access | Free |