In a groundbreaking study published in Physical Review Letters, researchers have developed a new method for simulating 3D morphology of kilonovae, the explosions of radiation that occur when two neutron stars collide. By modeling the 3D structure of the expanding debris, the team was able to successfully predict what the afterglow of a kilonova would look like. This could help astronomers better understand the physics behind these events and provide insight into the origin of heavy elements like gold and platinum.

Read Full Article Here

source: Phys.org