(M/R)1:(M/R)2=0.16:0.18

Detail

In this case, the two neutron stars have compactions $(M/R)$1$:(M/R)$2$=0.16:0.18$

Initial Configuration
Density and Magnetic Field Evolution
Gravitational Waveforms

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Illinois Relativity Group---University of Illinois at Urbana-Champaign

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Last Updated 22 June 2017 by EJC