Test of the statistical isotropy of the universe using gravitational waves
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Publication:5041307
DOI10.1088/1475-7516/2022/09/046OpenAlexW4295922452WikidataQ114824668 ScholiaQ114824668MaRDI QIDQ5041307
Sabino Matarrese, Angelo Ricciardone, Nicola Bartolo, Marina Migliaccio, Giacomo Galloni, Nicola Vittorio
Publication date: 13 October 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2202.12858
Relativistic cosmology (83F05) Signal detection and filtering (aspects of stochastic processes) (60G35) Quantum optics (81V80) Gravitational waves (83C35)
Related Items (4)
Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects ⋮ Galaxy number-count dipole and superhorizon fluctuations ⋮ GW_CLASS: Cosmological Gravitational Wave Background in the cosmic linear anisotropy solving system ⋮ An analytical study of the primordial gravitational-wave-induced contribution to the large-scale structure of the Universe
Uses Software
Cites Work
- NumPy
- Primordial gravity wave background anisotropies
- Anisotropies of gravitational wave backgrounds: a line of sight approach
- Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
- Cosmological backgrounds of gravitational waves
- Probing non-Gaussian stochastic gravitational wave backgrounds with LISA
- Cross-correlations as a diagnostic tool for primordial gravitational waves
- Gravitational waves and geometrical optics in scalar-tensor theories
- Testing the early universe with anisotropies of the gravitational wave background
- Gravitational wave anisotropies from primordial black holes
- Detecting the cosmic gravitational wave background with the Big Bang Observer
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