In an unstable Q-ball hairy black hole, the early growth of the weakly responding scalar component is dominated by a second-order QNM rather than its linear response.
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Model for cosmological formation of superheavy Q-balls from a broken scale invariance potential that may explain dark matter or early structure formation.
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Early-Time Nonlinear Growth in an Unstable Q-Ball Hairy Black Hole
In an unstable Q-ball hairy black hole, the early growth of the weakly responding scalar component is dominated by a second-order QNM rather than its linear response.
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Superheavy Q-Balls and Cosmology
Model for cosmological formation of superheavy Q-balls from a broken scale invariance potential that may explain dark matter or early structure formation.