chapters · 6
01Free Preview
Atomic Collision Course: When Atoms Become One
Understand fusion at the atomic level—how extreme heat makes atoms overcome repulsion and merge
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The Binding Energy Secret: Why Fusion Works
Discover the hidden curve that powers stars—and why iron is the universe's energy ceiling
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The Triple Challenge: Temperature, Density, Time
Learn why achieving fusion requires balancing three impossible conditions simultaneously
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Plasma: The Star Stuff
Explore the fourth state of matter that makes up 99% of the visible universe
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Magnetic Bottles & Laser Squeeze: Two Ways To Contain A Star
Compare magnetic confinement and inertial confinement—the two competing paths to fusion power
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The Q Factor: The Race To Breakeven
Understand how we measure fusion success—and why Q=1 is just the beginning
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