Difference between revisions of "Lyapunov-Schmidt equation"
Ulf Rehmann (talk | contribs) m (moved Lyapunov–Schmidt equation to Lyapunov-Schmidt equation: ascii title) |
Ulf Rehmann (talk | contribs) m (tex encoded by computer) |
||
Line 1: | Line 1: | ||
+ | <!-- | ||
+ | l0611501.png | ||
+ | $#A+1 = 21 n = 0 | ||
+ | $#C+1 = 21 : ~/encyclopedia/old_files/data/L061/L.0601150 Lyapunov\ANDSchmidt equation | ||
+ | Automatically converted into TeX, above some diagnostics. | ||
+ | Please remove this comment and the {{TEX|auto}} line below, | ||
+ | if TeX found to be correct. | ||
+ | --> | ||
+ | |||
+ | {{TEX|auto}} | ||
+ | {{TEX|done}} | ||
+ | |||
A non-linear integral equation of the form | A non-linear integral equation of the form | ||
− | + | $$ \tag{1 } | |
+ | u ( x) - \int\limits _ \Omega K ( x , s ) u ( s) d s = | ||
+ | $$ | ||
− | + | $$ | |
+ | = \ | ||
+ | U _ {01} \left ( \begin{array}{c} | ||
+ | x \\ | ||
+ | v | ||
+ | \end{array} | ||
+ | \right ) + \sum | ||
+ | _ { m+ } n\geq 2 U _ {mn} \left ( \begin{array}{c} | ||
+ | x \\ | ||
+ | u,v | ||
+ | \end{array} | ||
+ | \right ) ,\ x \in \Omega , | ||
+ | $$ | ||
where | where | ||
− | + | $$ | |
+ | U _ {01} \left ( \begin{array}{c} | ||
+ | x \\ | ||
+ | v | ||
+ | \end{array} | ||
+ | \right ) = K _ {0} ( x) v ( x) + \int\limits _ \Omega K _ {1} ( x , s ) v ( s) d s , | ||
+ | $$ | ||
− | + | $$ | |
+ | U _ {mn} \left ( \begin{array}{c} | ||
+ | x \\ | ||
+ | u,v | ||
+ | \end{array} | ||
+ | \right ) = \sum _ | ||
+ | {\nu = 1 } ^ { {n } } \int\limits _ \Omega \dots \int\limits _ \Omega | ||
+ | K ^ {(} v) ( x , s _ {1} \dots s _ {i} ) \times | ||
+ | $$ | ||
− | + | $$ | |
+ | \times u ^ {\alpha _ {0} } ( x) u ^ {\alpha _ {1} } ( s _ {1} ) \dots u ^ {\alpha _ {i} } ( s _ {i} ) v ^ {\beta _ {0} } ( x) v ^ {\beta _ {1} } ( s _ {1} ) \dots v ^ {\beta _ {i} } ( s _ {i} ) d s _ {1} \dots d s _ {i} , | ||
+ | $$ | ||
− | + | $ \alpha _ {0} \dots \alpha _ {i} $, | |
+ | $ \beta _ {0} \dots \beta _ {i} $ | ||
+ | are non-negative integers, | ||
− | + | $$ | |
+ | \alpha _ {0} + \dots + \alpha _ {i} = m ,\ \ | ||
+ | \beta _ {0} + \dots + \beta _ {i} = n , | ||
+ | $$ | ||
− | + | $ \Omega $ | |
+ | is a closed bounded set in a finite-dimensional Euclidean space, $ v $ | ||
+ | and the function $ K $ | ||
+ | are given continuous functions of their arguments, $ s _ {1} \dots s _ {i} \in \Omega $, | ||
+ | and $ u $ | ||
+ | is the unknown function. The sum on the right-hand side of (1) may be finite or it may represent an infinite series. In the latter case the series is called an integro-power series of two functional arguments. It is assumed that the series converges absolutely and uniformly. | ||
− | If 1 is not a characteristic number of the kernel | + | If 1 is not a characteristic number of the kernel $ K ( x , s ) $, |
+ | then equation (1) has a unique small solution in the class of continuous functions for sufficiently small $ | v ( x) | $. | ||
+ | This solution can be represented as an integro-power series. The case when 1 is a characteristic number of the kernel $ K $ | ||
+ | is more complicated. In this case one constructs a system of equations — the branching equations (bifurcation equations): | ||
− | + | $$ \tag{2 } | |
+ | \omega _ {k} ( \xi _ {1} \dots \xi _ {n} , v ) = 0 ,\ \ | ||
+ | k = 1 \dots n , | ||
+ | $$ | ||
− | where | + | where $ \omega _ {k} $ |
+ | are known power series and $ n $ | ||
+ | is the multiplicity of the characteristic number 1. In the general case the system (2) has a non-unique solution. Whatever the fixed sufficiently small function $ v $, | ||
+ | to every small continuous solution of (2) (a continuous solution of (2) is said to be small if $ \xi _ {i} ( 0) = 0 $) | ||
+ | there corresponds a small solution of (1) that can be represented as an integro-power series. | ||
An equation of the type (1) was first considered by A.M. Lyapunov in 1906, and later — in a more general form — by E. Schmidt in 1908. | An equation of the type (1) was first considered by A.M. Lyapunov in 1906, and later — in a more general form — by E. Schmidt in 1908. | ||
Line 29: | Line 91: | ||
====References==== | ====References==== | ||
<table><TR><TD valign="top">[1]</TD> <TD valign="top"> M.M. Vainberg, V.A. Trenogin, "Theory of branching of solutions of non-linear equations" , Noordhoff (1974) (Translated from Russian)</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top"> N.S. Smirnov, "Introduction to the theory of integral equations" , Moscow-Leningrad (1936) (In Russian)</TD></TR></table> | <table><TR><TD valign="top">[1]</TD> <TD valign="top"> M.M. Vainberg, V.A. Trenogin, "Theory of branching of solutions of non-linear equations" , Noordhoff (1974) (Translated from Russian)</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top"> N.S. Smirnov, "Introduction to the theory of integral equations" , Moscow-Leningrad (1936) (In Russian)</TD></TR></table> | ||
− | |||
− | |||
====Comments==== | ====Comments==== | ||
− | |||
====References==== | ====References==== | ||
<table><TR><TD valign="top">[a1]</TD> <TD valign="top"> S.-N. Chow, J.K. Hale, "Methods of bifurcation theory" , Springer (1982)</TD></TR></table> | <table><TR><TD valign="top">[a1]</TD> <TD valign="top"> S.-N. Chow, J.K. Hale, "Methods of bifurcation theory" , Springer (1982)</TD></TR></table> |
Latest revision as of 04:11, 6 June 2020
A non-linear integral equation of the form
$$ \tag{1 } u ( x) - \int\limits _ \Omega K ( x , s ) u ( s) d s = $$
$$ = \ U _ {01} \left ( \begin{array}{c} x \\ v \end{array} \right ) + \sum _ { m+ } n\geq 2 U _ {mn} \left ( \begin{array}{c} x \\ u,v \end{array} \right ) ,\ x \in \Omega , $$
where
$$ U _ {01} \left ( \begin{array}{c} x \\ v \end{array} \right ) = K _ {0} ( x) v ( x) + \int\limits _ \Omega K _ {1} ( x , s ) v ( s) d s , $$
$$ U _ {mn} \left ( \begin{array}{c} x \\ u,v \end{array} \right ) = \sum _ {\nu = 1 } ^ { {n } } \int\limits _ \Omega \dots \int\limits _ \Omega K ^ {(} v) ( x , s _ {1} \dots s _ {i} ) \times $$
$$ \times u ^ {\alpha _ {0} } ( x) u ^ {\alpha _ {1} } ( s _ {1} ) \dots u ^ {\alpha _ {i} } ( s _ {i} ) v ^ {\beta _ {0} } ( x) v ^ {\beta _ {1} } ( s _ {1} ) \dots v ^ {\beta _ {i} } ( s _ {i} ) d s _ {1} \dots d s _ {i} , $$
$ \alpha _ {0} \dots \alpha _ {i} $, $ \beta _ {0} \dots \beta _ {i} $ are non-negative integers,
$$ \alpha _ {0} + \dots + \alpha _ {i} = m ,\ \ \beta _ {0} + \dots + \beta _ {i} = n , $$
$ \Omega $ is a closed bounded set in a finite-dimensional Euclidean space, $ v $ and the function $ K $ are given continuous functions of their arguments, $ s _ {1} \dots s _ {i} \in \Omega $, and $ u $ is the unknown function. The sum on the right-hand side of (1) may be finite or it may represent an infinite series. In the latter case the series is called an integro-power series of two functional arguments. It is assumed that the series converges absolutely and uniformly.
If 1 is not a characteristic number of the kernel $ K ( x , s ) $, then equation (1) has a unique small solution in the class of continuous functions for sufficiently small $ | v ( x) | $. This solution can be represented as an integro-power series. The case when 1 is a characteristic number of the kernel $ K $ is more complicated. In this case one constructs a system of equations — the branching equations (bifurcation equations):
$$ \tag{2 } \omega _ {k} ( \xi _ {1} \dots \xi _ {n} , v ) = 0 ,\ \ k = 1 \dots n , $$
where $ \omega _ {k} $ are known power series and $ n $ is the multiplicity of the characteristic number 1. In the general case the system (2) has a non-unique solution. Whatever the fixed sufficiently small function $ v $, to every small continuous solution of (2) (a continuous solution of (2) is said to be small if $ \xi _ {i} ( 0) = 0 $) there corresponds a small solution of (1) that can be represented as an integro-power series.
An equation of the type (1) was first considered by A.M. Lyapunov in 1906, and later — in a more general form — by E. Schmidt in 1908.
References
[1] | M.M. Vainberg, V.A. Trenogin, "Theory of branching of solutions of non-linear equations" , Noordhoff (1974) (Translated from Russian) |
[2] | N.S. Smirnov, "Introduction to the theory of integral equations" , Moscow-Leningrad (1936) (In Russian) |
Comments
References
[a1] | S.-N. Chow, J.K. Hale, "Methods of bifurcation theory" , Springer (1982) |
Lyapunov-Schmidt equation. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Lyapunov-Schmidt_equation&oldid=22781