Abstract
Consider a system of differential equations:
where \( t \) represents the independent variable that we will call time and \( x_{1} ,x_{2} ,\; \ldots x_{n} \) the unknown functions, where \( X_{1} ,X_{2} , \ldots \,X_{n} \) are given functions of \( x_{1} ,x_{2} , \ldots \,x_{n} \). We suppose in general that the functions \( X_{1} ,X_{2} , \ldots \,X_{n} \) are analytic and one-to-one for all real values of \( x_{1} ,x_{2} , \ldots \,x_{n} \).
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Notes
- 1.
In my thesis, I did not state this restriction and I did not assume that the sum of the \( m \) was larger than 1. It would therefore seem that the theorem is incorrect when for example \( \lambda_{2} = \lambda_{1} \). This is not the case. If we had
$$ m_{2} \lambda_{2} + \cdots m_{n} \lambda_{n} = \lambda_{1} {\text{for }}\left( {m_{2} + m_{3} + \cdots m_{n} > 1} \right) $$some coefficients of the expansion would take the form \( A/0 \) and would become infinite. This is the reason why we had to assume that such a relationship does not hold. If on the other hand \( \lambda_{2} = \lambda_{1} \), then some coefficients would take the form \( 0/0 \).
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Poincaré, H. (2017). General Properties of the Differential Equations. In: The Three-Body Problem and the Equations of Dynamics. Astrophysics and Space Science Library, vol 443. Springer, Cham. https://doi.org/10.1007/978-3-319-52899-1_1
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DOI: https://doi.org/10.1007/978-3-319-52899-1_1
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