Numerical study of cusp formation on horizons in head-on non-spinning black hole mergers, with analysis of mass and multipole behavior at the cusp and a proposed phenomenological model.
It follows thatM in < M 1 +M 2 and moreover Min = (M 1 +M 2) s 1− 2M1M2 (M1 +M 2)2 = (M 1 +M 2) p 1−2η(24) withη=M 1M2/(M1 +M 2)2 being the symmetric mass ratio
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Cusp Formation in Merging Black Hole Horizons
Numerical study of cusp formation on horizons in head-on non-spinning black hole mergers, with analysis of mass and multipole behavior at the cusp and a proposed phenomenological model.