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• W3100294345 abstract "Two distinct perturbative approaches have been recently formulated within General Relativity, arguing for the screening of gravity in the ΛCDM Universe. In this paper we compare them and show that the offered screening concepts, each characterized by its own interaction range, can peacefully coexist. Accordingly, we advance a united scheme, determining the gravitational potential at all scales, including regions of nonlinear density contrasts, by means of a simple Helmholtz equation with the effective cosmological screening length. In addition, we claim that cosmic structures may not grow at distances above this Yukawa range and confront its current value with dimensions of the largest known objects in the Universe." @default.
• W3100294345 created "2020-11-23" @default.
• W3100294345 creator A5066885762 @default.
• W3100294345 creator A5074099476 @default.
• W3100294345 date "2020-09-01" @default.
• W3100294345 modified "2023-10-17" @default.
• W3100294345 title "Duel of cosmological screening lengths" @default.
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• W3100294345 doi "https://doi.org/10.1016/j.dark.2020.100565" @default.
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