Testing the distance duality relation using type Ia supernovae and ultracompact radio sources

Abstract

We test the possible deviation of the cosmic distance duality relation $D_A(z)(1+z{)}^2/D_L(z)\equiv 1$ using the standard candles/rulers in a fully model-independent manner. Type-Ia supernovae are used as the standard candles to derive the luminosity distance $D_L(z)$, and ultra-compact radio sources are used as the standard rulers to obtain the angular diameter distance $D_A(z)$. We write the deviation of distance duality relation as $D_A(z)(1+z{)}^2/D_L(z)=\eta (z)$. Specifically, we use two parameterizations of $\eta (z)$, i.e. ${\eta }_1(z)=1+{\eta }_{0}z$ and ${\eta }_2(z)=1+{\eta }_{0}z/(1+z)$. The parameter ${\eta }_0$ is obtained using the Markov chain Monte Carlo methods by comparing $D_L(z)$ and $D_A(z)$ at the same redshift. The best-fitting results are ${\eta }_0=-0.06\pm 0.05$ and $-0.18\pm 0.16$ for the first and second parameterizations, respectively. Our results depend on neither the cosmological models, nor the matter contents or the curvature of the universe.

6 pages, 4 figures, accepted by MNRAS

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• Is there a standard measuring rod in the Universe?