Anomalous decay rate of quasinormal modes

PHYSICAL REVIEW D 101:8 (2020) 84018

Authors:

Macarena Lagos, Pedro G Ferreira, Oliver J Tattersall

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)

Authors:

AP Lobban, TJ Turner, JN Reeves, V Braito, L Miller

LYACOLORE: synthetic datasets for current and future Lyman-alpha forest BAO surveys

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 2020:3 (2020) 68

Authors:

James Farr, Andreu Font-Ribera, Helion du Mas des Bourboux, Andrea Munoz-Gutierrez, F Javier Sanchez, Andrew Pontzen, Alma Xochitl Gonzalez-Morales, David Alonso, David Brooks, Peter Doel, Thomas Etourneau, Julien Guy, Jean-Marc Le Goff, Axel de la Macorra, Nathalie Palanque-Delabrouille, Ignasi Perez-Rafols, James Rich, ArCie Slosar, Gregory Tarle, Duan Yutong, Kai Zhang

Abstract:

© 2020 IOP Publishing Ltd and Sissa Medialab. The statistical power of Lyman-α forest Baryon Acoustic Oscillation (BAO) measurements is set to increase significantly in the coming years as new instruments such as the Dark Energy Spectroscopic Instrument deliver progressively more constraining data. Generating mock datasets for such measurements will be important for validating analysis pipelines and evaluating the effects of systematics. With such studies in mind, we present LyaCoLoRe: A package for producing synthetic Lyman-α forest survey datasets for BAO analyses. LyaCoLoRe transforms initial Gaussian random field skewers into skewers of transmitted flux fraction via a number of fast approximations. In this work we explain the methods of producing mock datasets used in LyaCoLoRe, and then measure correlation functions on a suite of realisations of such data. We demonstrate that we are able to recover the correct BAO signal, as well as large-scale bias parameters similar to literature values. Finally, we briefly describe methods to add further astrophysical effects to our skewers-high column density systems and metal absorbers-which act as potential complications for BAO analyses.

Why do extremely massive disc galaxies exist today?

(2020)

Authors:

Ryan A Jackson, Garreth Martin, Sugata Kaviraj, Clotilde Laigle, Julien Devriendt, Yohan Dubois, Christophe Pichon

Defining the Really Habitable Zone

(2020)

Authors:

Marven F Pedbost, Trillean Pomalgu, Chris Lintott, Nora Eisner, Belinda Nicholson