Stellar physics
How stars rotate, generate magnetic fields, evolve and leave compact remnants.
11 problemsStars, compact objects, and signals from space.
How stars rotate, generate magnetic fields, evolve and leave compact remnants.
11 problemsUnseen matter, cosmic expansion, energetic particles, and brief radio flashes.
40 problemsComposition, structure and internal dynamics of planets and stars.
37 problemsHow stars explode, what they leave behind, and where heavy elements form.
5 problemsBent light and galaxy motions reveal gravity that known stars and gas cannot fully explain. What supplies the additional mass?
If a black hole evaporates, how is the information about what fell into it represented in what comes out? The answer must reconcile quantum evolution with gravitational calculations.
Particles arrive at Earth with energies far beyond those reached by human accelerators. Which cosmic objects accelerate them, and by what process?
Brief radio flashes arrive from across the universe. Magnetars can produce some of them, but what generates their intense emission and explains the range of observed bursts?
The Sun’s outer atmosphere is much hotter than its visible surface. Which processes deliver and dissipate enough energy to maintain it?
Measurements of the Sun’s composition and interior do not all agree with standard solar models. Which changes would make the different lines of evidence fit together?