Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Himalaya Senapati"'
Publikováno v:
Resonance. 24:87-114
The classical three-body problem arose in an attempt to understand the effect of the Sun on the Moon's Keplerian orbit around the Earth. It has attracted the attention of some of the best physicists and mathematicians and led to the discovery of chao
Autor:
Himalaya Senapati
Publikováno v:
Eighteen Essays in Non-Euclidean Geometry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::323e22991c1ed9ef61835a8aa2d8df7e
https://doi.org/10.4171/196-1/4
https://doi.org/10.4171/196-1/4
Autor:
Himalaya Senapati
Publikováno v:
Eighteen Essays in Non-Euclidean Geometry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8b55c794025ea44c05e79ddfce14d33e
https://doi.org/10.4171/196-1/5
https://doi.org/10.4171/196-1/5
Autor:
Himalaya Senapati
Publikováno v:
Eighteen Essays in Non-Euclidean Geometry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9a0c16a24aef9e3eafb61329b498ac4e
https://doi.org/10.4171/196-1/6
https://doi.org/10.4171/196-1/6
Publikováno v:
Chaos: An Interdisciplinary Journal of Nonlinear Science. 30:043112
In the classical three rotor problem, three equal point masses move on a circle subject to attractive cosine potentials of strength g. In the center of mass frame, energy E is the only known conserved quantity. In earlier work [Krishnaswami and Senap
This paper concerns the classical dynamics of three coupled rotors: equal masses moving on a circle subject to attractive cosine inter-particle potentials. It is a simpler variant of the gravitational three-body problem and also arises as the classic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61c1aa3960ac166c3f61ae9343e84080