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May 25, 2026Open Access

P60: Rotational Stability of CCEGA Black Stars — Light Ring Damping Overwhelms Ergoregion Instability

Key Points

The research aims to establish the rotational stability of CCEGA black stars despite the effects of ergoregion instability.
Evaluated the damping rates of light rings and ergoregions for CCEGA black stars
Analyzed the effect of geometric factors on stability
Considered mass ranges from 4.56 to 14.75 M☉.
Light ring damping rate exceeds ergoregion instability rate by a factor of approximately 10⁹–10¹²
Rotational stability is confirmed for all evaluated masses
Geometric factors, notably (δr/r_e)⁵, play a crucial role in suppressing instability.

Abstract

We establish rotational stability of CCEGA black stars despite the ergoregion being exterior to the object (C ≈ 0. 63–1. 27, P51 v2. 0). The light ring damping rate exceeds the ergoregion instability rate by a factor γLR/γₑrgo ~ 10⁹–10¹². The suppression arises from geometric factors (δr/rₑ) ⁵ in the ergoregion-surface overlap. CCEGA black stars are rotationally stable for all masses in the range 4. 56–14. 75 M☉.

P60: Rotational Stability of CCEGA Black Stars — Light Ring Damping Overwhelms Ergoregion Instability

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Abstract

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