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Kwinten Fransen (KULeuven)03/11/2021, 16:10
Rotating black holes in general relativity are notoriously simple objects. They can be fully fixed by measuring a single dominant (complex) characteristic frequency. Having determined this 'quasinormal mode' (QNM) frequency for the endstate of a binary merger, any additional information, from earlier binary dynamics or other QNMs, can serve as a test of our understanding of general relativity...
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Daniel Mayerson03/11/2021, 16:30
Equatorial symmetry – flipping the sign of the z coordinate – is a somewhat accidental symmetry of the Kerr black hole. There is no theorem guaranteeing its existence for a stationary black hole, as opposed to axisymmetry. Indeed, in many string theory black holes and horizonless compact objects, equatorial symmetry is generically broken. Somehow surprisingly, however, the possible observable...
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Cristian Joana03/11/2021, 16:50
In this talk, I will motivate the usage of numerical relativity for studies on the early universe. In particular, I will show simulations of the preinflationary epoch to prove the robustness of Higgs inflation to inhomogeneous initial conditions. Also, I will show ongoing preliminary results: full GR simulation of the reheating, and investigations on primordial black hole formation during the...
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