Détail du document
Identifiant
oai:arXiv.org:2412.01219
Sujet
Astrophysics - Cosmology and Nonga... General Relativity and Quantum Cos... High Energy Physics - Phenomenolog...Auteur
Tian, Chi Ding, Ran Kou, Xiao-XiaoCatégorie
sciences : astrophysique
Année
2024
Date de référencement
04/12/2024
Mots clés
wave anisotropy bayesian gravitationalRésumé
We introduce a new method designed for Bayesian inference of the angular power spectrum of the Gravitational Wave Background (GWB) anisotropy.
This scheme works with time-series data and can optionally incorporate the cross-correlations between the GWB anisotropy and other cosmological tracers, enhancing the significance of Bayesian inference.
We employ the realistic LISA response and noise model to demonstrate the validity of this approach.
The findings indicate that, without considering any cross-correlations, the 4-year LISA data is insufficient to achieve a significant detection of multipoles.
However, if the anisotropies in the GWB are strongly correlated with the Cosmic Microwave Background (CMB), the 4-year data can provide unbiased estimates of the quadrupole moment ($\ell = 2$).
This reconstruction process is generic and not restricted to any specific detector, offering a new framework for extracting anisotropies in the GWB data from various current and future gravitational wave observatories.
;Comment: 11 pages, 4 figures
Tian, Chi,Ding, Ran,Kou, Xiao-Xiao, 2024, Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
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