Can we teach a machine to reproduce the physics of turbulence? An exploration of using deep learning to simulate magnetohydrodynamic turbulence!
The ‘mass gap’ is a mass range bereft of any observed neutron stars or black holes. What can gravitational waves tell us about possible inhabitants of this terra incognita?
What does the merger of a neutron star with a black hole look like? Here’s a systematic study of how neutron star properties affect the electromagnetic emission from the merger.
We know everything there is to know about the s-process, right? RIGHT?!
A look at how magnetic braking can erase the extended main sequence turn-off feature in old stellar clusters.