Late-time evolution of a self-interacting scalar field in the spacetime of a dilaton black hole
R. ModerskiNicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716 Warsaw, Bartycka 18, PolandMarek RogatkoNicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716 Warsaw, Bartycka 18, Poland
2001en
ABI
Abstract
We investigate the late-time tails of self-interacting (massive) scalar fields in the spacetime of a dilaton black hole. Following the no hair theorem we examine the mechanism by which self-interacting scalar hair decays. We reveal that the intermediate asymptotic behavior of the considered field perturbations is dominated by an oscillatory inverse power-law decaying tail. The numerical simulations show that at very late time, massive self-interacting scalar hair decays slower than any power law.
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