On Separate Universes
arXiv:1504.00351 · doi:10.1088/1475-7516/2015/10/059
Abstract
(abridged version) The separate universe conjecture states that in General Relativity a density perturbation behaves locally (i.e. on scales much smaller than the wavelength of the mode) as a separate universe with different background density and curvature. We prove this conjecture for a spherical compensated tophat density perturbation of arbitrary amplitude and radius in CDM. We then use Conformal Fermi Coordinates to generalize this result to scalar perturbations of arbitrary configuration and scale. In this case, the separate universe conjecture holds for the isotropic part of the perturbations. The anisotropic part on the other hand is exactly captured by a tidal field in the Newtonian form. We show that the separate universe picture is restricted to scales larger than the sound horizons of all fluid components. We then derive an expression for the locally measured matter bispectrum induced by a long-wavelength mode of arbitrary wavelength. We show that nonlinear gravitational dynamics does not generate observable contributions that scale like local-type non-Gaussianity , and hence does not contribute to a scale-dependent galaxy bias on large scales; rather, the locally measurable long-short mode coupling assumes a form essentially identical to subhorizon perturbation theory results, once the long-mode density perturbation is replaced by the synchronous-comoving gauge density perturbation. Apparent -type contributions arise through projection effects on photon propagation, which depend on the specific large-scale structure tracer and observable considered, and are in principle distinguishable from the local mode coupling induced by gravity. We conclude that any observation of beyond these projection effects signals a departure from standard single-clock inflation.
36 pages and 1 figure. To be submitted to JCAP. Comments are welcome. Version 2: Abstract improved. Added Section 5.2 to clarity the initial condition in CFC for single-clock inflation
References in corpus (10)
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- On the consistency relation of the 3-point function in single field inflation
- Conformal Symmetries of Adiabatic Modes in Cosmology
- Separate Universe Simulations
- Galaxy number counts to second order and their bispectrum
- Super-Sample Signal
- The angle-averaged squeezed limit of nonlinear matter N-point functions
- A Consistency Relation for the Observed Galaxy Bispectrum and the Local non-Gaussianity from Relativistic Corrections
- Einstein's signature in cosmological large-scale structure
- Galaxy bias and gauges at second order in General Relativity
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