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Higher order relativistic galaxy number counts: dominating terms

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arxiv 1606.02113 v3 pith:OLCBLTNL submitted 2016-06-07 astro-ph.CO gr-qc

classification astro-ph.COgr-qc
keywords ordertermscountsnumberhighercomparecomputeconcentrating
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We review the number counts to second order concentrating on the terms which dominate on sub horizon scales. We re-derive the result for these terms and compare it with the different versions found in the literature. We generalize our derivation to higher order terms, especially the third order number counts which are needed to compute the 1-loop contribution to the power spectrum.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Tetrad formalism for exact cosmological observables

    astro-ph.CO 2019-08 accept novelty 7.0 of 10

    The paper derives exact, coordinate-independent equations for cosmological observables on a new 'observer space-time' manifold, using tetrads to track the observer frame.

  2. Galaxy number counts at second order: an independent approach

    astro-ph.CO 2019-08 conditional novelty 5.0 of 10

    The authors present a new, independent derivation of the second-order relativistic galaxy number count in a flat expanding universe, but they only validate it at linear order against previous work.

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