On the nature of filaments of the large-scale structure of the Universe

Abstract : Observed properties of filaments which dominate in large-scale structure of the Universe are considered. A part from these properties isn't described within the standard ΛCDM cosmological model. The "toy" model of formation of primary filaments owing to the primary scalar and vector gravitational perturbations in the uniform and isotropic cosmological model which is filled with matter with negligible pressure, without use of a hypothesis of tidal interaction of dark matter halos is offered.
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https://hal.archives-ouvertes.fr/hal-01962100
Contributor : Irina Rozgacheva <>
Submitted on : Thursday, December 20, 2018 - 1:43:10 PM
Last modification on : Friday, December 21, 2018 - 4:20:21 PM
Long-term archiving on : Friday, March 22, 2019 - 11:10:05 AM

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  • HAL Id : hal-01962100, version 1

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Irina Rozgacheva, I Kuvshinova. On the nature of filaments of the large-scale structure of the Universe. 2018. ⟨hal-01962100⟩

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