How real-time cosmology can distinguish between different anisotropic models - INSPIRE

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How real-time cosmology can distinguish between different anisotropic models

Jul 9, 2013

25 pages

Published in:

JCAP 12 (2013) 042

Published: Dec 17, 2013

e-Print:

1307.2377 [astro-ph.CO]

DOI:

10.1088/1475-7516/2013/12/042

View in:

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Abstract: (IOP)

We present a new analysis on how to distinguish between isotropic and anisotropic cosmological models based on tracking the angular displacements of a large number of distant quasars over an extended period of time, and then performing a multipole-vector decomposition of the resulting displacement maps.We find that while the GAIA mission operating at its nominal specifications does not have sufficient angular resolution to resolve anisotropic universes from isotropic ones using this method within a reasonable timespan of ten years, a next-generation GAIA-like survey with a resolution ten times better should be equal to the task. Distinguishing between different anisotropic models is however more demanding. Keeping the observational timespan to ten years, we find that the angular resolution of the survey will need to be of order 0.1 μas in order for certain rotating anisotropic models to produce a detectable signature that is also unique to models of this class. However, should such a detectionbecome possible, it would immediately allow us to rule out large local void models.

Note:

25 pages, 4 figures; v2: 27 pages, 5 figures in new colour scheme, extended discussion on the uniqueness of the observer position, main conclusions unchanged, matches version accepted by JCAP

redshift surveys
cosmic ows
cosmological parameters from LSS

References(31)

Figures(15)

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