Cosmology
The expansion, history, and large-scale structure of the universe.
9 problemsMatter, energy, physical phenomena, and the universe.
The expansion, history, and large-scale structure of the universe.
9 problemsStars, compact objects, and signals from space.
28 problemsFundamental particles, interactions, and symmetries.
21 problemsQuantum phenomena and the foundations of their description.
11 problemsCollective behavior in materials and quantum matter.
17 problemsThe collective motion of gases, liquids, and charged matter.
8 problemsThe formation, interiors, and histories of planets and moons.
15 problemsEarth’s interior, geological history, and physical systems.
21 problemsFive open problems from Clay’s famous prize program, linking mathematics with computation and mathematical physics.
5 problemsUnseen matter, cosmic expansion, energetic particles, and brief radio flashes.
40 problemsMeasurement, gravity, and black holes challenge our account of quantum physics.
10 problemsBent light and galaxy motions reveal gravity that known stars and gas cannot fully explain. What supplies the additional mass?
The universe's expansion is accelerating. “Dark energy” names the gap in our explanation, while several different physical accounts remain possible.
Gravity describes a changing spacetime. Quantum physics describes matter and its possibilities. How should they work together in a single physical account?
The goal is a material that conducts electricity without resistance at room temperature and normal atmospheric pressure. Achieving both conditions together remains a research target.
Matter and antimatter can annihilate each other. Yet the observable universe contains enough leftover matter to make stars, planets, and people. What produced that imbalance?
The theory of the strong nuclear force permits a kind of asymmetry that experiments find to be extraordinarily small. Why is nature so close to the symmetric case?