scholarly journals Poisson geometry of PI three‐dimensional Sklyanin algebras

2018 ◽  
Vol 118 (6) ◽  
pp. 1471-1500
Author(s):  
Chelsea Walton ◽  
Xingting Wang ◽  
Milen Yakimov
Mathematics ◽  
2021 ◽  
Vol 9 (12) ◽  
pp. 1378
Author(s):  
Cristian Lăzureanu

In this paper we consider systems of three autonomous first-order differential equations x˙=f(x),x=(x,y,z),f=(f1,f2,f3) such that x(t)+y(t)+z(t) is constant for all t. We present some Hamilton–Poisson formulations and integrable deformations. We also analyze the case of Kolmogorov systems. We study from some standard and nonstandard Poisson geometry points of view the three-dimensional Lotka–Volterra system with constant population.


2021 ◽  
Vol 27 (5) ◽  
Author(s):  
Chelsea Walton ◽  
Xingting Wang ◽  
Milen Yakimov

2017 ◽  
Vol 16 (05) ◽  
pp. 1750085 ◽  
Author(s):  
Kevin De Laet

In this paper, it is shown how the Heisenberg group of order 27 can be used to construct quotients of degenerate Sklyanin algebras. These quotients have properties similar to the classical Sklyanin case in the sense that they have the same Hilbert series, the same character series and a central element of degree 3. Regarding the central element of a three-dimensional Sklyanin algebra, a better way to view this using Heisenberg-invariants is shown.


2004 ◽  
Vol 276 (2) ◽  
pp. 515-551 ◽  
Author(s):  
Koen de Naeghel ◽  
Michel van den Bergh

2017 ◽  
Vol 470 ◽  
pp. 379-419 ◽  
Author(s):  
Natalia Iyudu ◽  
Stanislav Shkarin

1966 ◽  
Vol 25 ◽  
pp. 227-229 ◽  
Author(s):  
D. Brouwer

The paper presents a summary of the results obtained by C. J. Cohen and E. C. Hubbard, who established by numerical integration that a resonance relation exists between the orbits of Neptune and Pluto. The problem may be explored further by approximating the motion of Pluto by that of a particle with negligible mass in the three-dimensional (circular) restricted problem. The mass of Pluto and the eccentricity of Neptune's orbit are ignored in this approximation. Significant features of the problem appear to be the presence of two critical arguments and the possibility that the orbit may be related to a periodic orbit of the third kind.


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