Implementation of gravitational potential screening on large scales in an N-body code
dc.contributor.author | Baldi, Marco | |
dc.contributor.author | Burgazli, Alvina | |
dc.contributor.author | Eingorn, Maxim | |
dc.contributor.author | Жук, Олександр Іванович | |
dc.contributor.author | Жук, Александр Иванович | |
dc.contributor.author | Zhuk, Oleksandr I. | |
dc.date.accessioned | 2020-02-20T13:27:30Z | |
dc.date.available | 2020-02-20T13:27:30Z | |
dc.date.issued | 2019 | |
dc.description.abstract | There was considered the Universe filled with cold dark matter in the form of discrete inhomogeneities (e.g., galax-ies) and dark energy in the form of arbitrary continuous per-fect fluids. The background space-time geometry is defined by the Friedmann metric. | uk_UA |
dc.identifier.citation | 6-th Gamow International Conference in Odessa "New trends in astrophysics, cosmology and hep after Gamow" and 19-th Gamow Summer School "Astronomy and beyond: astrophysics, cosmology, radioastronomy and astrobiology" (Ukraine, Odessa, Chernomorka, August 11-18, 2019) | uk_UA |
dc.identifier.uri | https://dspace.onu.edu.ua/handle/123456789/27251 | |
dc.language.iso | en | uk_UA |
dc.subject | the Universe | uk_UA |
dc.subject | dark energy | uk_UA |
dc.subject | N-body code | uk_UA |
dc.title | Implementation of gravitational potential screening on large scales in an N-body code | uk_UA |
dc.type | Article | uk_UA |
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