Matter Density and Gravitational Waves from Binary Neutron Star Merger

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Matter density and gravitational waves emitted from a binary neutron star merger, much like observed LIGO event, GW170817. Performed using the MAYA numerical relativity code.

Credit: Chris Evans, Bhavesh Khamesra, Deirdre Shoemaker, Pablo Laguna, Georgia Tech, MAYA Collaboration
  1. MAYA Collaboration
  2. Gravitational waves
  3. neutron stars
  4. GW170817
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It would be good to know what the visualisation of any matter not accreted would look like. Like would it remain in orbit, be thrown out, or slowly accrete back? This piques the imagination given that it is thought that this material is made up of all the cool elements.
Great modelling by the way and Thanks for posting.

aSpyIntheHaus