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Extreme Physics of Compact Objects: White Dwarfs, Neutron Stars, and Black Holes

Stellar Structure and Evolution → Gravitational Wave Emission

A graduate-level learning path that systematically builds from foundational physics to the extreme regimes of compact objects. It covers stellar evolution, degeneracy pressure, neutron star structure, pulsar magnetospheres, black hole thermodynamics, Hawking radiation, and gravitational wave emission, with necessary cross-domain links to general relativity, quantum mechanics, and statistical mechanics.

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11 steps · 11 nodes · 3 stages

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11 nodes14 edges1 relationships

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Path Steps

11 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

4 steps

Stage 2

Core Concepts

4 steps

Stage 3

Advanced Topics

3 steps

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