Zero Tidal Deformability of Black Holes Does not Prove The Singularity

Kriger B.
2026.
Why black holes probably have no measurable tidal deformability and why that does not imply a singularity.
IIIR Cosmology and Theoretical Physics.
This scientific paper argues that black holes lack measurable tidal deformability a conclusion that aligns with standard general relativity but does not necessitate the existence of a central singularity.
The author demonstrates that a frozen star model featuring a uniform vacuum core also predicts a vanishing tidal Love number because its exterior remains a perfect vacuum.
Through a reanalysis of gravitational-wave data the study confirms that current observations are consistent with these predictions across different theoretical frameworks.
Consequently the paper formally withdraws previous claims that supermassive black holes would exhibit detectable tidal signatures in the future.
Instead the author identifies Kgr-Radiation a specific continuous gravitational-wave signal as the only definitive way to distinguish between a singular interior and a regular vacuum core.
This radiation is expected to occur at predictable frequencies relative to an objects mass providing a sharp test for next-generation detectors like LISA. Kriger B.
2026.
Why black holes probably have no measurable tidal deformability and why that does not imply a singularity.
IIIR Cosmology and Theoretical Physics.

Источник: rutube.ru