title: Rigid body rotation in relativistic approximation
metadata.name: dc.contributor.author
metadata.value: Pashkevich, Vladimir V.
metadata.lang: -
metadata.name: dc.date.accessioned
metadata.value: 2018-09-18T11:56:53Z
metadata.lang: -
metadata.name: dc.date.available
metadata.value: 2018-09-18T11:56:53Z
metadata.lang: -
metadata.name: dc.date.issued
metadata.value: 2018-09
metadata.lang: -
metadata.name: dc.identifier.citation
metadata.value: Pashkevich V.V. Rigid body rotation in relativistic approximation. Vestnik of Saint Petersburg University. Mathematics. Mechanics. Astronomy, 2018, vol. 5 (63), issue 3, pp. 494–508.
metadata.lang: en_GB
metadata.name: dc.identifier.other
metadata.value: 10.21638/11701/spbu01.2018.313
metadata.lang: -
metadata.name: dc.identifier.uri
metadata.value: http://hdl.handle.net/11701/14892
metadata.lang: -
metadata.name: dc.description.abstract
metadata.value: In this research, relativistic rotation of a rigid body, which is generated by metric properties
  of Riman space of general relativity, is studied. The main purpose of this investigation
  is to obtain Lagrange function for the relativistic rotation of a rigid body. In order to
  attain this aims the whole system of point masses mi, in which a certain set of point
  masses dmn forms an “absolutely rigid body” mn in such a way that the condition of a
  constant distance between any two point masses from the set of point masses dmn holds,
  was investigated. In this case, the body mn can rotate around its own center of mass
  with angular velocity |ω| ≥ 0. The remaining point masses mj from the set mi are point
  bodies, which do not rotate. Lagrange function for the relativistic rotation of a rigid body
  is deriving from Lagrange function of the non-rotation point of masses system in the postnewtonian
  approximation.
metadata.lang: en_GB
metadata.name: dc.description.sponsorship
metadata.value: Работа выполнена при финансовой поддержке в рамках сотрудничества между ЦКИ ПАН
  и ГАО РАН и персональных грантов Александра Бжезиньского и Иоланты Настулы.
metadata.lang: en_GB
metadata.name: dc.language.iso
metadata.value: ru
metadata.lang: en_GB
metadata.name: dc.publisher
metadata.value: St Petersburg State University
metadata.lang: en_GB
metadata.name: dc.relation.ispartofseries
metadata.value: Vestnik of St Petersburg University. Mathematics. Mechanics. Astronomy;Volume 5(63); Issue 3
metadata.lang: -
metadata.name: dc.subject
metadata.value: rigid body rotation
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: Lagrange function
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: Riman space
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: general relativity
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: postnewtonian approximation
metadata.lang: en_GB
metadata.name: dc.title
metadata.value: Rigid body rotation in relativistic approximation
metadata.lang: en_GB
metadata.name: dc.type
metadata.value: Article
metadata.lang: en_GB
resources.filename: 13-Pashkevich.pdf
resources.url: https://dspace.spbu.ru/bitstream/11701/14892/1/13-Pashkevich.pdf
resources.format: Adobe PDF
resources.size: 450,33 kB