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Black Hole Remnants from BH-NS Mergers by Piero Tokunaga is a document available to read on EtoBox.
What is Black Hole Remnants from BH-NS Mergers about?
1) Black hole-neutron star mergers may soon be observed through gravitational waves and electromagnetic counterparts. These mergers result in a remnant black hole that depends on the properties of the coalescing binary. 2) Using numerical relativity simulations, the authors construct a map from binary parameters like mass ratio, black hole spin, and neutron star equation of state to the properties of the remnant black hole. 3) By combining this with population synthesis models, they predict the masses o
- Author
- Piero Tokunaga
- Language
- EN