2014/11/30 by Vakhid A. Gani, Alexander E. Dmitriev, Sergey G. Rubin
Physics and Astronomy · #Class (philosophy) #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Domain (mathematical analysis) #Extra dimensions #Galaxies: Formation, Evolution, Phenomena #Parameter space #Scattering #Space (punctuation) #Space time #astro-ph.CO #gr-qc #hep-th
paper · pdf · doi:10.1142/s0218271815450017
published as Int. J. Mod. Phys. D 24, 1545001 (2015) · 12 pages, 5 figures; V2: some changes to match version published in IJMPD
openalex publication_date 2015/07/13 · arxiv created 2015/09/19 · openalex created_date 2016/06/24 · arxiv updated 2016/11/24 · openalex updated_date 2026/08/05
We elaborate the possibility for a deformed extra space to be considered as the dark matter candidate. To perform calculations, a class of two-dimensional extra metrics was considered in the framework of the multidimensional gravity. It was shown that there exists a family of stationary metrics of the extra space possessing point-like defect. Estimation of cross-section of scattering of a particle of the ordinary matter on a spatial domain with deformed extra space is in agreement with the observational constraints.