2020
DOI: 10.1093/mnras/staa1936
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The failure of testing for cosmic opacity via the distance-duality relation

Abstract: Abstract The distance-duality relation (DDR) between the luminosity distance DL and the angular diameter distance DA is viewed as a powerful tool for testing for the opacity of the Universe, being independent of any cosmological model. It was applied by many authors, who mostly confirm its validity and report a negligible opacity of the Universe. Nevertheless, a thorough analysis reveals that applying the DDR in cosmic opacity tests is tricky. Its applicability i… Show more

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Cited by 11 publications
(11 citation statements)
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“…Yet, interestingly, the HII region data favors a transition from τ = 0 at low redshift to τ > 0 at higher redshift, a behavior that is consistent with the true optical depth increasing with redshifts. Such tendency, which is different from that obtained in the framework of parameterized form, is supported by the recent works of Ma & Corasaniti (2018); Vavryčuk & Kroupa (2020) stressing the importance of cosmic-opacity test without a prescribed phenomenological function.…”
Section: Methodology and Constrained Results Of Cosmic Opacitymentioning
confidence: 83%
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“…Yet, interestingly, the HII region data favors a transition from τ = 0 at low redshift to τ > 0 at higher redshift, a behavior that is consistent with the true optical depth increasing with redshifts. Such tendency, which is different from that obtained in the framework of parameterized form, is supported by the recent works of Ma & Corasaniti (2018); Vavryčuk & Kroupa (2020) stressing the importance of cosmic-opacity test without a prescribed phenomenological function.…”
Section: Methodology and Constrained Results Of Cosmic Opacitymentioning
confidence: 83%
“…Considering the fact that X-ray photons can destroy dust grains instead of being absorbed, physically different processes could be detected from the observations of X-ray fluxes, instead of simple luminosity dimming due to dust absorption of low-energy photons (Draine & Hao 2002;Morgan et al 2014). Our final results showed that the cosmic opacity could attain different values for different types of D L data covering different wavelengths (optical for HII regions, SNe Ia Pantheon sample, ultraviolet for quasar sample), although such effect is still difficult to be precisely quantified (see Vavryčuk & Kroupa (2020) for a detailed discussion). Thus, the goal of our test is not just to check the resolution power of the GW data, but also to assess the performance of the combination of current and future available data in gravitational wave (GW) and electromagnetic (EM) domain.…”
Section: Conclusion and Discussionmentioning
confidence: 91%
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