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Quarks to Cosmos

How Feynman Diagrams Saved Physics

26 min2 april 2026

Our everyday intuition suggests that empty space should be weightless, as there is seemingly "nothing" there; however, gravity measurements reveal that the vacuum actually holds a significant amount of energy or mass.

In the early 1980s, Richard Feynman grappled with this "weight of nothing," seeking to understand why the vacuum—the region with the lowest possible energy—seems to weigh practically nothing.

To understand this, one must distinguish between a "vacuum," where particles and fluctuations are removed, and the theoretical "void," which lacks any physical properties whatsoever—a concept that has evolved from Newton's "empty stage" to the modern understanding of quantum fields.

Feynman diagrams revolutionized this field by providing a visual and mathematical shorthand for the complex interactions within quantum fields, where particles like electrons and photons emerge as localized disturbances.

While these diagrams streamlined theories like Quantum Electrodynamics (QED) and are now generated by the thousands using AI and graph neural networks to handle complex calculations, they did not fully solve the mystery of the vacuum’s weight.

Quantum fields introduce troublesome infinities, especially when calculating gravity, and although Feynman hoped his diagrams would bypass these issues by describing interactions directly, the challenge of reconciling the weight of empty space remains a fundamental frontier in physics.

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