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General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

We extend the general relativistic description of galaxy clustering developed in Yoo, Fitzpatrick, and Zaldarriaga (2009). For the first time we provide a fully general relativistic description of the observed matter power spectrum and the observed galaxy power spectrum with the linear bias ansatz. It is significantly different from the standard Newtonian description on large scales and especially its measurements on large scales can be misinterpreted as the detection of the primordial non-Gaussianity even in the absence thereof. The key difference in the observed galaxy power spectrum arises from the real-space matter fluctuation defined as the matter fluctuation at the hypersurface of the observed redshift. As opposed to the standard description, the shape of the observed galaxy power spectrum evolves in redshift, providing additional cosmological information. While the systematic errors in the standard Newtonian description are negligible in the current galaxy surveys at low redshift, correct general relativistic description is essential for understanding the galaxy power spectrum measurements on large scales in future surveys with redshift depth z>3. We discuss ways to improve the detection significance in the current galaxy surveys and comment on applications of our general relativistic formalism in future surveys.

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astro-ph.CO 3

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2026 3

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representative citing papers

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges

astro-ph.CO · 2026-05-06 · unverdicted · novelty 7.0 · 2 refs

A Newtonian Motion Gauge found via Einstein-Boltzmann solver maps linear dynamics with scale-dependent growth and GR corrections to Newtonian equations, enabling consistent nonlinear EFT calculations that are transformed back for accuracy in real and redshift space.

Relativistic effects in k-essence

astro-ph.CO · 2026-04-22 · unverdicted · novelty 4.0

Relativistic effects dominate large-scale galaxy power spectra and grow with redshift, but are largely insensitive to k-essence microphysics in Fourier space while the angular spectrum shows clearer model distinctions, especially for the tachyon.

citing papers explorer

Showing 3 of 3 citing papers.

  • Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges astro-ph.CO · 2026-05-06 · unverdicted · none · ref 44 · 2 links · internal anchor

    A Newtonian Motion Gauge found via Einstein-Boltzmann solver maps linear dynamics with scale-dependent growth and GR corrections to Newtonian equations, enabling consistent nonlinear EFT calculations that are transformed back for accuracy in real and redshift space.

  • The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects astro-ph.CO · 2026-05-28 · accept · none · ref 37 · internal anchor

    Fourier transforming over observer positions yields a diagonal power spectrum for any lightcone observable, from which standard two-point and higher-order statistics follow as projections.

  • Relativistic effects in k-essence astro-ph.CO · 2026-04-22 · unverdicted · none · ref 8

    Relativistic effects dominate large-scale galaxy power spectra and grow with redshift, but are largely insensitive to k-essence microphysics in Fourier space while the angular spectrum shows clearer model distinctions, especially for the tachyon.