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Model of the Newtonian cosmology: Symmetries, invariant and partialy invariant solutions / I. Klebanova,c, , O. Startsuna, S. Ivanovb
dc.contributor.author | Klebanov, Igor | |
dc.contributor.author | Startsun, O. | |
dc.contributor.author | Ivanov, S. | |
dc.contributor.author | Клебанов, Игорь Иосифович | |
dc.date.accessioned | 2015-06-05T09:20:18Z | |
dc.date.available | 2015-06-05T09:20:18Z | |
dc.date.issued | 2015-06-05 | |
dc.identifier.uri | http://elib.cspu.ru/xmlui/handle/123456789/663 | |
dc.description.abstract | Symmetry group of the equation system of ideal nonrelativistic self-gravitating fluid with zero pressure is calculated. Submodel invariant under the sub-group of rotations SO(3) is built and symmetry group of the factorsystem is calculated. A particular analytical invariant solution of the factorsystem is obtained. | ru_RU |
dc.language.iso | en | ru_RU |
dc.subject | Newtonian cosmology | ru_RU |
dc.subject | Ideal self-gravitating | ru_RU |
dc.subject | Lie point symmetries | ru_RU |
dc.subject | Invariant solutions | ru_RU |
dc.title | Model of the Newtonian cosmology: Symmetries, invariant and partialy invariant solutions / I. Klebanova,c, , O. Startsuna, S. Ivanovb | ru_RU |
dc.title.alternative | препринт статьи для журнала "Cosmology" | ru_RU |
dc.type | Preprint | ru_RU |