Anomalous decay rate of quasinormal modes
PHYSICAL REVIEW D 101:8 (2020) 84018
Abstract:
© 2020 American Physical Society. The decay timescales of the quasinormal modes of a massive scalar field have an intriguing behavior: they either grow or decay with increasing angular harmonic numbers ℓ, depending on whether the mass of the scalar field is small or large. We identify the properties of the effective potential of the scalar field that leads to this behavior and characterize it in detail. If the scalar field is nonminimally coupled, considered here, the scalar quasinormal modes will leak into the gravitational wave signal and will have decaying times that are comparable or smaller than those typical in general relativity. Hence, these modes could be detectable in the future. Finally, we find that the anomalous behavior in the decay timescales of quasinormal modes is present in a much larger class of models beyond a simple massive scalar field.X-ray variability analysis of a large series of XMM-Newton + NuSTAR observations of NGC 3227
ArXiv 2004.03824 (2020)
LYACOLORE: synthetic datasets for current and future Lyman-alpha forest BAO surveys
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 2020:3 (2020) 68