The failure of testing for cosmic opacity via the distance-duality relation

被引:8
|
作者
Vavrycuk, Vaclav [1 ]
Kroupa, Pavel [2 ,3 ]
机构
[1] Czech Acad Sci, Inst Geophys, Bocni 2, CZ-14100 Prague 4, Czech Republic
[2] Univ Bonn, Helmholtz Inst Strahlen & Kemphys, Nussallee 14-16, D-53115 Bonn, Germany
[3] Charles Univ Prague, Astron Inst, Fac Math & Phys, V Holesovickach 2, CZ-18000 Prague 8, Czech Republic
关键词
gravitational lensing: strong; opacity; supernovae: general; galaxies: clusters: general; intergalactic medium; dark energy; SIZE REDSHIFT RELATION; GAMMA-RAY BURSTS; INTERGALACTIC DUST; DARK ENERGY; INTERSTELLAR DUST; BACKGROUND-RADIATION; UNIVERSE OPACITY; GALAXY CLUSTERS; IA; CONSTRAINTS;
D O I
10.1093/mnras/staa1936
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The distance-duality relation (DDR) between the luminosity distance D-L and the angular diameter distance D-A 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 is strongly limited because of a non-unique interpretation of the D-L data in terms of cosmic opacity and a rather low accuracy and deficient extent of currently available D-A data. Moreover, authors usually assume that cosmic opacity is frequency independent and parametrize it in their tests by a prescribed phenomenological function. In this way, they only prove that cosmic opacity does not follow their assumptions. As a consequence, no convincing evidence of transparency of the universe using the DDR has so far been presented.
引用
收藏
页码:378 / 388
页数:11
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