Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-16572
Marinoni, C; Saintonge, A; Giovanelli, R; Haynes, M P; Masters, K L; LeFévre, O; Mazure, A; Taxil, P; Virey, J M (2008). Geometrical tests of cosmological models. I. Probing dark energy using the kinematics of high redshift galaxies. Astronomy and Astrophysics, 478(1):43-55.
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We suggest to use the observationally measured and theoretically justified correlation between size and rotational velocity of galactic discs as a viable method to select a set of high redshift standard rods which may be used to explore the dark energy content of the universe via the classical angular-diameter test. Here we explore a new strategy for an optimal implementation of this test.We propose to use the rotation speed of high redshift galaxies as a standard size indicator and show how high resolution multi-object spectroscopy and ACS/HST high quality spatial images, may be combined to measure the amplitude of the dark energy density parameter ΩQ, or to constrain the cosmic equation of state parameter for a smooth dark energy component (w = p/ρ, −1 ≤ w < −1/3). Nearly 1300 standard rods with high velocity rotation in the bin V = 200 ± 20 km s−1 are expected in a field of 1 sq. degree and over the
redshift baseline 0 < z < 1.4. This sample is sufficient to constrain the cosmic equation of state parameter w at a level of 20% (without priors in the [Ωm,ΩQ] plane) even when the [OII]λ3727 Å linewidth-diameter relationship is calibrated with a scatter of ∼40%. We evaluate how systematics may affect the proposed tests, and find that a linear standard rod evolution, causing galaxy dimensions
to be up to 30% smaller at z = 1.5, can be uniquely diagnosed, and will minimally bias the confidence level contours in the [ΩQ, w] plane. Finally, we show how to derive, without a priori knowing the specific functional form of disc evolution, a cosmologyevolution diagram with which it is possible to establish a mapping between different cosmological models and the amount of galaxy
disc/luminosity evolution expected at a given redshift.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute of Theoretical Physics|
|Uncontrolled Keywords:||cosmology: observations -- cosmology: theory -- cosmology: cosmological parameters -- galaxies: high-redshift -- galaxies: fundamental parameters -- galaxies: evolution|
|Deposited On:||11 Mar 2009 17:15|
|Last Modified:||27 Nov 2013 19:18|
|Citations:||Web of Science®. Times cited: 3|
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