Implementation of gravitational potential screening on large scales in an N-body code

dc.contributor.authorBaldi, Marco
dc.contributor.authorBurgazli, Alvina
dc.contributor.authorEingorn, Maxim
dc.contributor.authorЖук, Олександр Іванович
dc.contributor.authorЖук, Александр Иванович
dc.contributor.authorZhuk, Oleksandr I.
dc.date.accessioned2020-02-20T13:27:30Z
dc.date.available2020-02-20T13:27:30Z
dc.date.issued2019
dc.description.abstractThere 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.citation6-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.urihttps://dspace.onu.edu.ua/handle/123456789/27251
dc.language.isoenuk_UA
dc.subjectthe Universeuk_UA
dc.subjectdark energyuk_UA
dc.subjectN-body codeuk_UA
dc.titleImplementation of gravitational potential screening on large scales in an N-body codeuk_UA
dc.typeArticleuk_UA
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