Ultra-relativistic black hole flybys can radiate over 65% of their energy in gravitational waves via irregular waveforms caused by radiation trapping and lensing, without coalescence.
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An analytic model with no free parameters predicts 13.8% of initial energy radiated as gravitational waves for light-speed head-on equal-mass black hole collisions.
Fifth RIT catalog adds 248 new binary black hole waveforms emphasizing eccentric orbits with convergence studies on 10 simulations, reaching 2129 total cases.
citing papers explorer
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Trapping, Irregular Waveforms, and Efficient Radiation in Ultra-relativistic Black Hole Encounters
Ultra-relativistic black hole flybys can radiate over 65% of their energy in gravitational waves via irregular waveforms caused by radiation trapping and lensing, without coalescence.
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Gravitational Wave Energy Emitted in the Head-On Collision of Two Black Holes
An analytic model with no free parameters predicts 13.8% of initial energy radiated as gravitational waves for light-speed head-on equal-mass black hole collisions.
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The Fifth RIT Catalog of Binary Black Hole Simulations: Multiple-Resolution Studies of Eccentric Orbits
Fifth RIT catalog adds 248 new binary black hole waveforms emphasizing eccentric orbits with convergence studies on 10 simulations, reaching 2129 total cases.