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Neyrinck, Szapudi & Szalay (2009)

San Diego State University

The big idea

As structure grows non-linear, the matter power spectrum Pδ(k)P_\delta(k) becomes a bad summary statistic: gravitational evolution couples Fourier modes, the late-time density is dominated by a few sharp peaks (haloes), and the cosmological information that was cleanly held in the linear power spectrum leaks into higher-order statistics and into a large, “translinear” covariance. Neyrinck, Szapudi & Szalay show that a single, simple operation undoes much of this damage: replace δ\delta with the log-density log(1+δ)\log(1+\delta) before measuring the power spectrum.

The log-mapped power spectrum Plog(1+δ)(k)P_{\log(1+\delta)}(k) has a shape “hardly departing from the linear power spectrum for k1hMpc1k \lesssim 1\,h\,\mathrm{Mpc}^{-1} at all redshifts,” and — the headline — recovers pristine Fisher information, yielding about 10× more cumulative signal-to-noise at z=0z=0 than the standard power spectrum over a range of scales.

Why it works

The density field is statistically invariant under translations and rotations; all the cosmological information of the Gaussian initial conditions lives in the power spectrum, with every higher moment zero. Non-linear growth breaks this by making the one-point PDF non-Gaussian (δ\delta develops a long tail and a hard floor at δ=1\delta=-1). Because the late-time PDF is approximately lognormal (Coles & Jones (1991)), restoring Gaussianity to the one-point distribution — by taking the log — pulls the strayed information back into the two-point function. Phase correlations (which build genuine cosmic-web filaments) affect higher-order statistics but not the power spectrum, so a monotone one-point remap recovers what it can without needing the phases.

Use in progenax

Notes

References
  1. Neyrinck, M. C., Szapudi, I., & Szalay, A. S. (2009). Rejuvenating the Matter Power Spectrum: Restoring Information with a Logarithmic Density Mapping. The Astrophysical Journal Letters, 698, L90–L93. 10.1088/0004-637X/698/2/L90