Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data
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Abstract
We use the latest baryon acoustic oscillation and Union 2.1 type Ia supernova data to test the cosmic opacity between different redshift regions without assuming any cosmological models. It is found that the universe may be opaque between the redshift regions 0.35–0.44, 0.44–0.57 and 0.6–0.73 since the best fit values of cosmic opacity in these regions are positive, while a transparent universe is favored in the redshift region 0.57–0.63. However, in general, a transparent universe is still consistent with observations at the 1\sigma confidence level.
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He-Kun Li, Pu-Xun Wu, Hong-Wei Yu. Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data[J]. Chin. Phys. Lett., 2016, 33(5): 059801. DOI: 10.1088/0256-307X/33/5/059801
He-Kun Li, Pu-Xun Wu, Hong-Wei Yu. Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data[J]. Chin. Phys. Lett., 2016, 33(5): 059801. DOI: 10.1088/0256-307X/33/5/059801
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He-Kun Li, Pu-Xun Wu, Hong-Wei Yu. Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data[J]. Chin. Phys. Lett., 2016, 33(5): 059801. DOI: 10.1088/0256-307X/33/5/059801
He-Kun Li, Pu-Xun Wu, Hong-Wei Yu. Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data[J]. Chin. Phys. Lett., 2016, 33(5): 059801. DOI: 10.1088/0256-307X/33/5/059801
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