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A class of surfaces and curves that have quite good smoothness properties; it was introduced in potential theory by A.M. Lyapunov at the turn into the 20th century.
 
A class of surfaces and curves that have quite good smoothness properties; it was introduced in potential theory by A.M. Lyapunov at the turn into the 20th century.
  
A surface <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611901.png" /> in the three-dimensional Euclidean space <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611902.png" /> is called a Lyapunov surface if it satisfies the following three conditions (Lyapunov's conditions): 1) at every point of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611903.png" /> there is a well-defined tangent plane, and consequently a well-defined normal; 2) there is a number <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611904.png" />, the same for all points of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611905.png" />, such that if one takes the part <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611906.png" /> of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611907.png" /> lying inside the Lyapunov sphere <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611908.png" /> with centre at an arbitrary point <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l0611909.png" /> and radius <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119010.png" />, then the lines parallel to the normal to <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119011.png" /> at <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119012.png" /> meet <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119013.png" /> at most once; and 3) there are two numbers <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119014.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119015.png" />, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119016.png" />, the same for the whole of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119017.png" />, such that for any two points <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119018.png" />,
+
A surface $  S $
 +
in the three-dimensional Euclidean space $  \mathbf R  ^ {3} $
 +
is called a Lyapunov surface if it satisfies the following three conditions (Lyapunov's conditions): 1) at every point of $  S $
 +
there is a well-defined tangent plane, and consequently a well-defined normal; 2) there is a number $  r > 0 $,  
 +
the same for all points of $  S $,  
 +
such that if one takes the part $  \Sigma $
 +
of $  S $
 +
lying inside the Lyapunov sphere $  B ( y _ {0} , r ) $
 +
with centre at an arbitrary point $  y _ {0} \in S $
 +
and radius $  r $,  
 +
then the lines parallel to the normal to $  S $
 +
at $  y _ {0} $
 +
meet $  \Sigma $
 +
at most once; and 3) there are two numbers $  A > 0 $
 +
and $  \lambda $,
 +
0 < \lambda \leq  1 $,  
 +
the same for the whole of $  S $,  
 +
such that for any two points $  y _ {1} , y _ {2} \in S $,
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119019.png" /></td> <td valign="top" style="width:5%;text-align:right;">(*)</td></tr></table>
+
$$ \tag{* }
 +
| \theta |  < A  | y _ {1} - y _ {2} |  ^  \lambda  ,
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119020.png" /> is the angle between the normals to <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119021.png" /> at <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119022.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119023.png" />. Sometimes these three conditions are supplemented by the requirement that <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119024.png" /> is closed and that the solid angle under which any part <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119025.png" /> of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119026.png" /> is visible at an arbitrary point <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119027.png" /> is uniformly bounded.
+
where $  \theta $
 +
is the angle between the normals to $  S $
 +
at $  y _ {1} $
 +
and $  y _ {2} $.  
 +
Sometimes these three conditions are supplemented by the requirement that $  S $
 +
is closed and that the solid angle under which any part $  \sigma $
 +
of $  S $
 +
is visible at an arbitrary point $  x \in \mathbf R  ^ {3} $
 +
is uniformly bounded.
  
The Lyapunov conditions can be generalized to hypersurfaces in <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119028.png" />, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119029.png" />.
+
The Lyapunov conditions can be generalized to hypersurfaces in $  \mathbf R  ^ {n} $,  
 +
$  n \geq  3 $.
  
Similarly, a simple continuous curve <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119030.png" /> in the plane <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119031.png" /> is called a Lyapunov curve if it satisfies the following conditions: <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119032.png" />) at every point of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119033.png" /> there is a well-defined tangent, and consequently a well-defined normal; and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119034.png" />) there are two numbers <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119035.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119036.png" />, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119037.png" />, the same for the whole of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119038.png" />, such that for any two points <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119039.png" /> (*) holds, where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119040.png" /> is the angle between the tangents or normals to <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119041.png" /> at <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119042.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119043.png" />. Here Lyapunov's condition 2) follows from <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119044.png" />) and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119045.png" />). The Lyapunov curves are a subclass of the simple smooth curves.
+
Similarly, a simple continuous curve $  L $
 +
in the plane $  \mathbf R  ^ {2} $
 +
is called a Lyapunov curve if it satisfies the following conditions: $  1  ^  \prime  $)  
 +
at every point of $  L $
 +
there is a well-defined tangent, and consequently a well-defined normal; and $  3  ^  \prime  $)  
 +
there are two numbers $  A > 0 $
 +
and $  \lambda $,
 +
0 < \lambda \leq  1 $,  
 +
the same for the whole of $  L $,  
 +
such that for any two points $  y _ {1} , y _ {2} \in L $(*)  
 +
holds, where $  \theta $
 +
is the angle between the tangents or normals to $  L $
 +
at $  y _ {1} $
 +
and $  y _ {2} $.  
 +
Here Lyapunov's condition 2) follows from $  1  ^  \prime  $)  
 +
and $  3  ^  \prime  $).  
 +
The Lyapunov curves are a subclass of the simple smooth curves.
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  A.M. Lyapunov,  "On certain questions connected with the Dirichlet problem" , ''Collected works'' , '''1''' , Moscow  (1954)  pp. 45–47; 48–100  (In Russian)</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top">  S.L. Sobolev,  "Partial differential equations of mathematical physics" , Pergamon  (1964)  (Translated from Russian)</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top">  V.S. Vladimirov,  "Equations of mathematical physics" , MIR  (1984)  pp. Chapt. 5  (Translated from Russian)</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top">  N.I. Muskhelishvili,  "Singular integral equations" , Wolters-Noordhoff  (1972)  pp. Chapt. 1  (Translated from Russian)</TD></TR></table>
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  A.M. Lyapunov,  "On certain questions connected with the Dirichlet problem" , ''Collected works'' , '''1''' , Moscow  (1954)  pp. 45–47; 48–100  (In Russian)</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top">  S.L. Sobolev,  "Partial differential equations of mathematical physics" , Pergamon  (1964)  (Translated from Russian)</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top">  V.S. Vladimirov,  "Equations of mathematical physics" , MIR  (1984)  pp. Chapt. 5  (Translated from Russian)</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top">  N.I. Muskhelishvili,  "Singular integral equations" , Wolters-Noordhoff  (1972)  pp. Chapt. 1  (Translated from Russian)</TD></TR></table>
 
 
  
 
====Comments====
 
====Comments====
A Lyapunov surface is necessarily <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119046.png" />, and on the other hand a compact surface of class <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l061/l061190/l06119047.png" /> is a Lyapunov surface. Lyapunov surfaces are used in the study of simple- and double-layer potentials.
+
A Lyapunov surface is necessarily $  C  ^ {1} $,  
 +
and on the other hand a compact surface of class $  C  ^ {2} $
 +
is a Lyapunov surface. Lyapunov surfaces are used in the study of simple- and double-layer potentials.

Latest revision as of 04:11, 6 June 2020


A class of surfaces and curves that have quite good smoothness properties; it was introduced in potential theory by A.M. Lyapunov at the turn into the 20th century.

A surface $ S $ in the three-dimensional Euclidean space $ \mathbf R ^ {3} $ is called a Lyapunov surface if it satisfies the following three conditions (Lyapunov's conditions): 1) at every point of $ S $ there is a well-defined tangent plane, and consequently a well-defined normal; 2) there is a number $ r > 0 $, the same for all points of $ S $, such that if one takes the part $ \Sigma $ of $ S $ lying inside the Lyapunov sphere $ B ( y _ {0} , r ) $ with centre at an arbitrary point $ y _ {0} \in S $ and radius $ r $, then the lines parallel to the normal to $ S $ at $ y _ {0} $ meet $ \Sigma $ at most once; and 3) there are two numbers $ A > 0 $ and $ \lambda $, $ 0 < \lambda \leq 1 $, the same for the whole of $ S $, such that for any two points $ y _ {1} , y _ {2} \in S $,

$$ \tag{* } | \theta | < A | y _ {1} - y _ {2} | ^ \lambda , $$

where $ \theta $ is the angle between the normals to $ S $ at $ y _ {1} $ and $ y _ {2} $. Sometimes these three conditions are supplemented by the requirement that $ S $ is closed and that the solid angle under which any part $ \sigma $ of $ S $ is visible at an arbitrary point $ x \in \mathbf R ^ {3} $ is uniformly bounded.

The Lyapunov conditions can be generalized to hypersurfaces in $ \mathbf R ^ {n} $, $ n \geq 3 $.

Similarly, a simple continuous curve $ L $ in the plane $ \mathbf R ^ {2} $ is called a Lyapunov curve if it satisfies the following conditions: $ 1 ^ \prime $) at every point of $ L $ there is a well-defined tangent, and consequently a well-defined normal; and $ 3 ^ \prime $) there are two numbers $ A > 0 $ and $ \lambda $, $ 0 < \lambda \leq 1 $, the same for the whole of $ L $, such that for any two points $ y _ {1} , y _ {2} \in L $(*) holds, where $ \theta $ is the angle between the tangents or normals to $ L $ at $ y _ {1} $ and $ y _ {2} $. Here Lyapunov's condition 2) follows from $ 1 ^ \prime $) and $ 3 ^ \prime $). The Lyapunov curves are a subclass of the simple smooth curves.

References

[1] A.M. Lyapunov, "On certain questions connected with the Dirichlet problem" , Collected works , 1 , Moscow (1954) pp. 45–47; 48–100 (In Russian)
[2] S.L. Sobolev, "Partial differential equations of mathematical physics" , Pergamon (1964) (Translated from Russian)
[3] V.S. Vladimirov, "Equations of mathematical physics" , MIR (1984) pp. Chapt. 5 (Translated from Russian)
[4] N.I. Muskhelishvili, "Singular integral equations" , Wolters-Noordhoff (1972) pp. Chapt. 1 (Translated from Russian)

Comments

A Lyapunov surface is necessarily $ C ^ {1} $, and on the other hand a compact surface of class $ C ^ {2} $ is a Lyapunov surface. Lyapunov surfaces are used in the study of simple- and double-layer potentials.

How to Cite This Entry:
Lyapunov surfaces and curves. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Lyapunov_surfaces_and_curves&oldid=47731
This article was adapted from an original article by E.D. Solomentsev (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article