Answers are grounded in this paper and cite their sources.
Interactions of high-density matter with rapidly rotating black holes are a natural outcome of core collapse in massive stars, neutron star mergers, or the coalescence of black hole-neutron star binaries. An ensuing long-lived state of suspended accretion may explain GRB 030329/SN 2003dh and GRB 060614. It predicts a chirp in gravitational radiation with exponential decaying frequency, by correlation of the radius of the surrounding matter with an expanding ISCO during viscous relaxation to a nearly Schwarzschild spacetime. The asymptotic value f gw (in kHz) provides novel metrology of the black hole mass M ⩽ 5.9 f −1 gw M ☉ . An optimal search algorithm is included.
No takes yet. Share an insight, caveat, or question.
Maurice H. P. M. van Putten (2008) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: