Towards investigation of evolution of dynamical systems with independence of time accuracy: more classes of systems View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2015-07

AUTHORS

V. G. Gurzadyan, A. A. Kocharyan

ABSTRACT

The recently developed method (Paper 1) enabling one to investigate the evolution of dynamical systems with an accuracy not dependent on time is developed further. The classes of dynamical systems which can be studied by that method are much extended, now including systems that are: (1) non-Hamiltonian, conservative; (2) Hamiltonian with time-dependent perturbation; (3) non-conservative (with dissipation). These systems cover various types of N-body gravitating systems of astrophysical and cosmological interest, such as the orbital evolution of planets, minor planets, artificial satellites due to tidal, non-tidal perturbations and thermal thrust, evolving close binary stellar systems, and the dynamics of accretion disks. More... »

PAGES

332

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1140/epjc/s10052-015-3560-0

DOI

http://dx.doi.org/10.1140/epjc/s10052-015-3560-0

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1013969193


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