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- W2004123789 abstract "One of the fundamental hypotheses in observational cosmology is the validity of the so-called cosmic distance-duality relation. In this paper, we perform Monte Carlo simulations based on the method developed in Holanda, Gonifmmode mbox{c{c}}else c{c}fi{}alves, and Alcaniz [J. Cosmol. Astropart. Phys. 06 (2012) 022] to answer the following question: what is the number of galaxy clusters observations ${N}_{text{crit}}$ needed to check the validity of this relation at a given confidence level? At $2ensuremath{sigma}$, we find that ${N}_{text{crit}}$ should be increased at least by a factor of 5 relative to the current sample size if we assume the current observational uncertainty ${ensuremath{sigma}}_{text{obs}}$. Reducing this latter quantity by a factor of 2, we show that the present amount of data would be already close to the required number to check the validity of the cosmic distance-duality relation at $2ensuremath{sigma}$." @default.
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- W2004123789 date "2015-01-27" @default.
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- W2004123789 title "Forecasting constraints on the cosmic duality relation with galaxy clusters" @default.
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- W2004123789 doi "https://doi.org/10.1103/physrevd.91.027302" @default.
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