Dipole of the luminosity distance: a direct measure of H(z)

Details Dipole of the luminosity distance: a direct measure of H(z) Dipole of the luminosity distance: a direct measure of H(z)

2006-03-09

arxiv.org/abs/astro-ph/0603240v3

Phys.Rev.Lett. 96 (2006) 191302

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, minor changes, matches published version

Scientific paper

10.1103/PhysRevLett.96.191302

We show that the dipole of the luminosity distance is a useful observational tool which allows us to determine the Hubble parameter as a function of the redshift H(z). We determine the number of supernovae needed to achieve a given precision for H(z) and to distinguish between different models for dark energy. We analyse a sample of nearby supernovae and find a dipole consistent with the cosmic microwave background at a significance of more than 2 sigma.

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