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Spherically symmetric gravitational collapse of a dust cloud in third order Lovelock Gravity

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arxiv 1107.2730 v1 pith:GFINTB3Z submitted 2011-07-14 gr-qc

classification gr-qc
keywords ordercollapsegravitationallovelocknakedsingularitiesspace-timecase
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abstract

We investigate the spherically symmetric gravitational collapse of an incoherent dust cloud by considering a LTB type space-time in third order Lovelock Gravity without cosmological constant, and give three families of LTB-like solutions which separately corresponding to hyperbolic, parabolic and elliptic. Notice that the contribution of high order curvature corrections have a profound influence on the nature of the singularity, and the global structure of space-time changes drastically from the analogous general relativistic case. Interestingly, the presence of high order Lovelock terms leads to the formation of massive, naked and time-like singularities in the 7D space-time, which is disallowed in general relativity. Moveover, we point out that the naked singularities in the 7D case may be gravitational weak therefore may not be a serious threat to the cosmic censorship hypothesis, while the naked singularities in the $D\geq8$ inhomogeneous collapse violate the cosmic censorship hypothesis seriously.

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  1. Higher Lovelock Curvature Terms Favor Local Nakedness in Dust Collapse

    gr-qc 2026-06 unverdicted novelty 7.0 of 10

    Higher Lovelock orders promote local visibility of central shell-focusing singularities in dust collapse by controlling the apparent horizon formation relative to the singularity curve.

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