2015/11/30 by Hong-Ming Zhu, Ue-Li Pen, Ue‐Li Pen +3 · 3 citations
Physics and Astronomy · #Anisotropy #Astrophysics #COSMIC cancer database #Computational physics #Correlation function (quantum field theory) #Cosmic microwave background #Cosmology and Gravitation Theories #Field (mathematics) #Galaxies: Formation, Evolution, Phenomena #Isotropy #Optics #Physics #Quantum mechanics #Radio Astronomy Observations and Technology #Scale (ratio) #Wavelength #astro-ph.CO
paper · pdf · doi:10.1103/physrevd.93.103504
published as Phys. Rev. D 93, 103504 (2016) · 12 pages, 8 figures, published version
openalex publication_date 2016/05/04 · arxiv created 2017/12/22 · arxiv updated 2017/12/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The gravitational coupling of a long-wavelength tidal field with small-scale density fluctuations leads to anisotropic distortions of the locally measured small-scale matter correlation function. Since the local correlation function is known to be statistically isotropic in the absence of such tidal interactions, the tidal distortions can be used to reconstruct the long-wavelength tidal field and large-scale density field in analogy with the cosmic microwave background lensing reconstruction. In this paper we present the theoretical framework of cosmic tidal reconstruction and test the reconstruction in numerical simulations. We find that the density field on large scales can be reconstructed with good accuracy and the cross-correlation coefficient between the reconstructed density field and the original density field is greater than 0.9 on large scales (k\ensuremath\lesssim0.1 h/Mpc), with the filter scale \ensuremath∼1.25 Mpc/h. This is useful in the 21 cm intensity mapping survey, where the long-wavelength radial modes are lost due to a foreground subtraction process.