We construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for current and future ground-based experiments, as well as for planned space missions. We present our results in a language similar to that used in cosmic microwave background and intensity mapping experiments, and connect the formalism with the sensitivity curves that are common lore in GWB analyses.

Alonso, D., Contaldi, C., Cusin, G., Ferreira, P., Renzini, A. (2020). Noise angular power spectrum of gravitational wave background experiments. PHYSICAL REVIEW D, 101(12) [10.1103/PhysRevD.101.124048].

Noise angular power spectrum of gravitational wave background experiments

Renzini A. I.
2020

Abstract

We construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for current and future ground-based experiments, as well as for planned space missions. We present our results in a language similar to that used in cosmic microwave background and intensity mapping experiments, and connect the formalism with the sensitivity curves that are common lore in GWB analyses.
Articolo in rivista - Articolo scientifico
gravitational wave
English
2020
101
12
124048
open
Alonso, D., Contaldi, C., Cusin, G., Ferreira, P., Renzini, A. (2020). Noise angular power spectrum of gravitational wave background experiments. PHYSICAL REVIEW D, 101(12) [10.1103/PhysRevD.101.124048].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/459299
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