Recently, many gravitational wave events from compact binary mergers have been detected by LIGO. Determining the final mass and spin of the remnant black holes (RBHs) is a fundamental issue and is also important in astrophysics.Unified models for predicting the final mass and spin of the RBHs from compact binary mergers is proposed.
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View Code? Open in Web Editor NEWTo calculate the mass and spin of the remnant black hole/Neutron star from a binary system merger. Based on the equations given by Deng Can-Min
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