Detecting the relativistic bispectrum in 21cm intensity maps
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Publication:5028761
DOI10.1088/1475-7516/2021/06/039zbMath1485.83027arXiv2009.06197OpenAlexW3084656448MaRDI QIDQ5028761
Chris Clarkson, Sheean Jolicoeur, Obinna Umeh, Roy Maartens, Stefano Camera, Eline M. de Weerd
Publication date: 10 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2009.06197
Signal detection and filtering (aspects of stochastic processes) (60G35) Diffraction, scattering (78A45) Electromagnetic fields in general relativity and gravitational theory (83C50)
Related Items (2)
Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum ⋮ Including relativistic and primordial non-Gaussianity contributions in cosmological simulations by modifying the initial conditions
Uses Software
Cites Work
- Large-scale galaxy bias
- Observed galaxy number counts on the light cone up to second order: III. Magnification bias
- Imprints of local lightcone \ projection effects on the galaxy bispectrum. Part II
- Imprints of local lightcone projection effects on the galaxy bispectrum. Part III. Relativistic corrections from nonlinear dynamical evolution on large-scales
- Non-Gaussianities due to relativistic corrections to the observed galaxy bispectrum
- A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
- Imprint of non-linear effects on HI intensity mapping on large scales
- Full-sky bispectrum in redshift space for 21cm intensity maps
- Detecting the relativistic galaxy bispectrum
- The relativistic dipole and gravitational redshift on LSS
- CLASS
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