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It is argued that the quantum of area between consecutive, high overtones quasinormal modes of a black hole horizon coincides with the area gap predicted by Loop Quantum Gravity, as… Click to show full abstract
It is argued that the quantum of area between consecutive, high overtones quasinormal modes of a black hole horizon coincides with the area gap predicted by Loop Quantum Gravity, as long as the horizon is isolated and the Barbero-Immirzi parameter is $\gamma \approx \sqrt{3}/6$, in agreement with the value derived from the Bekenstein-Hawking horizon entropy.
Keywords:
area;
loop quantum;
quantum gravity;
quasinormal modes;
modes horizon
Journal Title: General Relativity and Gravitation
Year Published: 2022
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Journal Title: General Relativity and Gravitation
Year Published: 2022
Link to full text (if available)
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recommendations!