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Testing cosmic opacity from SNe Ia and Hubble parameter through three cosmological-model-independent methods
We use the newly published 28 observational Hubble parameter data ()
and current largest SNe Ia samples (Union2.1) to test whether the universe is
transparent. Three cosmological-model-independent methods (nearby SNe Ia
method, interpolation method and smoothing method) are proposed through
comparing opacity-free distance modulus from Hubble parameter data and
opacity-dependent distance modulus from SNe Ia . Two parameterizations,
and are adopted for the
optical depth associated to the cosmic absorption. We find that the results are
not sensitive to the methods and parameterizations. Our results support a
transparent universe.Comment: 11 pages, 8 figures, 1 table, PLB(in press
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