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2015

Tidal Forces in Naked Singularity Backgrounds

Goel, Akash, Maity, Reevu, Roy, Pratim et al.

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The end stage of a gravitational collapse process can generically result in a black hole or a naked singularity.

Here we undertake a comparative analysis of the nature of tidal forces in these backgrounds.
The effect of such forces is generically exemplified by the Roche limit, which predicts the distance within which a celestial object disintegrates due to the tidal effects of a second more massive object.
In this paper, using Fermi normal coordinates, we numerically compute the Roche limit for a class of non-rotating naked singularity backgrounds, and compare them with known results for Schwarzschild black holes.

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