Quasinormal modes and horizon area quantisation in Loop Quantum Gravity
نویسندگان
چکیده
It is argued that the quantum of area between consecutive, high overtones quasinormal modes a black hole horizon coincides with gap predicted by Loop Quantum Gravity, as long isolated and Barbero-Immirzi parameter $\gamma \approx \sqrt{3}/6$, in agreement value derived from Bekenstein-Hawking entropy.
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ژورنال
عنوان ژورنال: General Relativity and Gravitation
سال: 2022
ISSN: ['0001-7701', '1572-9532']
DOI: https://doi.org/10.1007/s10714-022-02905-8