Gravitational collapse in pure Gauss–Bonnet theory

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The study shows that a central singularity forms under various initial conditions in gravitational collapse.
Initial matter configurations include dust and fluids with viscosity, affecting the time and nature of singularity formation.
Black hole horizons are formed and evolve based on the gravitational dynamics of the matter fields initially considered.
Central singularity remains hidden from observers at infinity, highlighting the intricate nature of gravitational effects.

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Analysis explores black hole horizon formation in gravitational collapse of matter fields, indicating hidden singularities.

Kumar et al. (2025) studied this question.

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