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Regular Keplerian motions in classical many-body systems. / Butikov, Eugene I.

In: European Journal of Physics, Vol. 21, No. 5, 01.09.2000, p. 465-482.

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Butikov, Eugene I. / Regular Keplerian motions in classical many-body systems. In: European Journal of Physics. 2000 ; Vol. 21, No. 5. pp. 465-482.

BibTeX

@article{ca5adfdb35354f298be87bfbc6ec6c56,
title = "Regular Keplerian motions in classical many-body systems",
abstract = "A clear and simple physical approach to the explanation of exact particular solutions of the classical many-body problem is suggested. When the motion of individual bodies coupled by mutual gravitational forces in a many-body system occurs along conic sections, each body can be treated as moving not under the pull of the other moving bodies, but rather under a stationary central inverse-square gravitational field. These solutions describing possible amazingly simple (Keplerian) many-body motions are illustrated by computer simulations. Some pedagogical and philosophical aspects of the problem are discussed.",
author = "Butikov, {Eugene I.}",
year = "2000",
month = sep,
day = "1",
doi = "10.1088/0143-0807/21/5/313",
language = "English",
volume = "21",
pages = "465--482",
journal = "European Journal of Physics",
issn = "0143-0807",
publisher = "IOP Publishing Ltd.",
number = "5",

}

RIS

TY - JOUR

T1 - Regular Keplerian motions in classical many-body systems

AU - Butikov, Eugene I.

PY - 2000/9/1

Y1 - 2000/9/1

N2 - A clear and simple physical approach to the explanation of exact particular solutions of the classical many-body problem is suggested. When the motion of individual bodies coupled by mutual gravitational forces in a many-body system occurs along conic sections, each body can be treated as moving not under the pull of the other moving bodies, but rather under a stationary central inverse-square gravitational field. These solutions describing possible amazingly simple (Keplerian) many-body motions are illustrated by computer simulations. Some pedagogical and philosophical aspects of the problem are discussed.

AB - A clear and simple physical approach to the explanation of exact particular solutions of the classical many-body problem is suggested. When the motion of individual bodies coupled by mutual gravitational forces in a many-body system occurs along conic sections, each body can be treated as moving not under the pull of the other moving bodies, but rather under a stationary central inverse-square gravitational field. These solutions describing possible amazingly simple (Keplerian) many-body motions are illustrated by computer simulations. Some pedagogical and philosophical aspects of the problem are discussed.

UR - http://www.scopus.com/inward/record.url?scp=0347316329&partnerID=8YFLogxK

U2 - 10.1088/0143-0807/21/5/313

DO - 10.1088/0143-0807/21/5/313

M3 - Article

AN - SCOPUS:0347316329

VL - 21

SP - 465

EP - 482

JO - European Journal of Physics

JF - European Journal of Physics

SN - 0143-0807

IS - 5

ER -

ID: 51954830