Graviton mass might reduce tension between early and late time cosmological data
Graviton mass might reduce tension between early and late time cosmological data
复制标题
引力子质量可能会减少早期和晚期宇宙学数据之间的紧张关系
DOI:
10.1103/physrevlett.118.091104
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发表时间:
2017
影响因子:
8.6
通讯作者:
A. De Felice and S. Mukohyama
中科院分区:
文献类型:
--
作者:
Y.Namekawa;渡邉和宏,藤井宏次;A. De Felice and S. Mukohyama
The standard cold dark matter model with a cosmological constant (-CDM) predicts a growth of structures which tends to be higher than the values of redshift space distortion (RSD) measurements if the cosmological parameters are fixed by the cosmic microwave background data. In this Letter, we point out that this discrepancy can be resolved or understood if we assume that the graviton has a small but nonzero mass. In the context of the minimal theory of massive gravity (MTMG), due to infrared Lorentz violations measurable only at present cosmological scales, the graviton acquires a mass without being haunted by unwanted extra degrees of freedom. While the so-called self-accelerating branch of cosmological solutions in the MTMG has the same phenomenology for the background as well as the scalar- and vector-type linear perturbations as thein general relativity (GR), it is possible to choose another branch so that the background is the same as that in GR, but the evolution of matter perturbations gets modified by the graviton mass. In studying the fit of such modified dynamics to the above-mentioned RSD measurements, we find that themodel is less probable than the MTMG by 2 orders of magnitude. With the help of the cross-correlation between the integrated Sachs-Wolfe effect and the large-scale structure, the data also pin down the graviton mass squared around, which is consistent with the latest boundset by the recent LIGO observation.