The study of hyper-accreting black holes and the origin of gold in the Universe

Project: Research project

Project Details

Description

The recent discovery of the first binary neutron star merger observed over the
electromagnetic spectrum and gravitational waves revealed exciting insights
on the formation of heavy elements in the Universe. By coupling numerical
simulation to observations, we can better understand the behavior of compact
objects, and how they merge. This proposal is focused on developing a
numerical code and using it to perform novel simulations that will dramatically
advance our understanding of the properties of these signals and how heavy
elements, such as gold and platinum are created. With the results from the
simulations, we can inform observational surveys about where to look for the
emission from the heavy elements in the thermal emission from the merger.
This proposal is also aimed to use observational data from the non-thermal
afterglow in order to constrain properties from the binary neutron star merger
itself.
StatusActive
Effective start/end date8/1/218/31/24

Funding

  • Space Telescope Science Institute (HST-HF2-51487.001-A//NAS5- 26555)
  • National Aeronautics and Space Administration (HST-HF2-51487.001-A//NAS5- 26555)

Fingerprint

Explore the research topics touched on by this project. These labels are generated based on the underlying awards/grants. Together they form a unique fingerprint.