Dipole of the luminosity distance as a test for dark energy models

Abstract

The dependence of Hubble parameter on redshift can be determined directly from the dipole of luminosity distance to Supernovae Ia. We investigate the possibility of using the data on dipole of the luminosity distance obtained from the Supernovae Ia compilations SDSS, Union2.1, JLA and Pantheon to distinguish the dark energy models.

arXiv comment4 pages, 4 figures, 2 tables

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