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- W3045753678 abstract "We explore the covariance of redshift-space matter power spectra after a standard density-field reconstruction. We derive perturbative formula of the covariance at the tree-level order and find that the amplitude of the off-diagonal components from the trispectrum decreases by reconstruction. Using a large set of $N$-body simulations, we also find the similar reduction of the off-diagonal components of the covariance and thereby the signal-to-noise ratio (S/N) of the postreconstructed (postrec) power spectra significantly increases compared to the prereconstructed spectra. This indicates that the information leaking to higher-order statistics come back to the two-point statistics by reconstruction. Interestingly, the postrec spectra have higher S/N than the linear spectrum with Gaussian covariance when the scale of reconstruction characterized with the smoothing scale of the shift field is below $ensuremath{sim}10text{ }text{ }{h}^{ensuremath{-}1}text{ }mathrm{Mpc}$ where the trispectrum becomes negative. We demonstrate that the error of the growth rate estimated from the monopole and quadrupole components of the redshift-space matter power spectra significantly improves by reconstruction. We also find a similar improvement of the growth rate even when taking into account the supersample covariance, while the reconstruction cannot correct for the field variation of the supersample modes." @default.
- W3045753678 created "2020-08-03" @default.
- W3045753678 creator A5039316110 @default.
- W3045753678 creator A5067428193 @default.
- W3045753678 creator A5070095293 @default.
- W3045753678 date "2020-10-09" @default.
- W3045753678 modified "2023-10-18" @default.
- W3045753678 title "Covariance of the redshift-space matter power spectrum after reconstruction" @default.
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- W3045753678 doi "https://doi.org/10.1103/physrevd.102.083514" @default.
- W3045753678 hasPublicationYear "2020" @default.
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