A new observable signature from frame-dragging processes near spinning black holes enables testing Einstein gravity and spin measurement via X-ray polarimetry.
Astrophysical Black Holes,
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Quantizing geodesic motion of dust particles in rotating black hole geometries produces many-body ground states whose core size and effective interior geometry depend on angular momentum.
citing papers explorer
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A New Method for Testing Einstein's Theory of Gravity Close to Rapidly Spinning Black Holes
A new observable signature from frame-dragging processes near spinning black holes enables testing Einstein gravity and spin measurement via X-ray polarimetry.
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Quantum dust cores of rotating black holes
Quantizing geodesic motion of dust particles in rotating black hole geometries produces many-body ground states whose core size and effective interior geometry depend on angular momentum.