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''principle of stationary action''
 
''principle of stationary action''
  
 
A variational integral principle in the dynamics of holonomic systems restricted by ideal stationary constraints and occurring under the action of potential forces that do not explicitly depend on time.
 
A variational integral principle in the dynamics of holonomic systems restricted by ideal stationary constraints and occurring under the action of potential forces that do not explicitly depend on time.
  
According to Lagrange's principle, in a real motion of a holonomic system for which the energy integral <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572001.png" /> exists, between a certain initial position <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572002.png" /> and a final position <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572003.png" />, the Lagrange action
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According to Lagrange's principle, in a real motion of a holonomic system for which the energy integral $  T + V = h $
 +
exists, between a certain initial position $  A _ {0} $
 +
and a final position $  A _ {1} $,  
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the Lagrange action
  
<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/l057/l057200/l0572004.png" /></td> </tr></table>
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$$
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\int\limits _ {t _ {0} } ^ { t }  2 T  dt  = \int\limits _ {A _ {0} } ^ { {A } _ {1} } \sum _  \nu  m _  \nu  v _  \nu  \cdot d r _  \nu  $$
  
has a stationary value in comparison with the kinematically possible motions between these positions with the same energy <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572005.png" /> as in the real motion. Here <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572006.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572007.png" /> are the kinetic and the potential energy of the system, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572008.png" /> is the amount of motion (momentum) of the <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l0572009.png" />-th point of the system and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l05720010.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l05720011.png" /> are the instants when the system passes through the positions <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l05720012.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057200/l05720013.png" />.
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has a stationary value in comparison with the kinematically possible motions between these positions with the same energy $  h $
 +
as in the real motion. Here $  T $
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and $  V $
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are the kinetic and the potential energy of the system, $  m _  \nu  v _  \nu  $
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is the amount of motion (momentum) of the $  \nu $-
 +
th point of the system and $  t _ {0} $
 +
and $  t $
 +
are the instants when the system passes through the positions $  A _ {0} $
 +
and $  A _ {1} $.
  
 
If the initial and final positions of the system are sufficiently close to one another, then the Lagrange action has a minimum for a real motion; in this connection the Lagrange principle is also called the principle of least action in Lagrange's form.
 
If the initial and final positions of the system are sufficiently close to one another, then the Lagrange action has a minimum for a real motion; in this connection the Lagrange principle is also called the principle of least action in Lagrange's form.
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====References====
 
====References====
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  P.L.M. Maupertuis,  ''Histoire l'Acad. Royale Sci. Paris 1744''  (1748)  pp. 417</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top">  L. Euler,  "Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes sive solutio problematis isoperimetrici latissimo sensu accepti" , Lausanne-Geneva  (1744)</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top">  J.L. Lagrange,  "Essai d'une nouvelle méthode pour déterminer les maxima et les minima des formules intégrales indéfinies"  J.A. Serret (ed.) , ''Oeuvres'' , '''1''' , G. Olms, reprint  (1973)  pp. 333–362</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top">  G.K. Suslov,  "Theoretical mechanics" , Moscow  (1944)  (In Russian)</TD></TR></table>
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  P.L.M. Maupertuis,  ''Histoire l'Acad. Royale Sci. Paris 1744''  (1748)  pp. 417</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top">  L. Euler,  "Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes sive solutio problematis isoperimetrici latissimo sensu accepti" , Lausanne-Geneva  (1744)</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top">  J.L. Lagrange,  "Essai d'une nouvelle méthode pour déterminer les maxima et les minima des formules intégrales indéfinies"  J.A. Serret (ed.) , ''Oeuvres'' , '''1''' , G. Olms, reprint  (1973)  pp. 333–362</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top">  G.K. Suslov,  "Theoretical mechanics" , Moscow  (1944)  (In Russian)</TD></TR></table>
 
 
  
 
====Comments====
 
====Comments====
 
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  V.I. Arnol'd,  "Mathematical methods of classical mechanics" , Springer  (1978)  (Translated from Russian)</TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top">  E.T. Whittaker,  "Analytical dynamics of particles and rigid bodies" , Dover, reprint  (1944)</TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top">  F.R. [F.R. Gantmakher] Gantmacher,  "Lectures in analytical mechanics" , MIR  (1975)  (Translated from Russian)</TD></TR><TR><TD valign="top">[a4]</TD> <TD valign="top">  J.L. Lagrange,  "Mécanique analytique" , '''1–2''' , Blanchard, reprint , Paris  (1965)  ((Also: Oeuvres, Vol. 11.))</TD></TR></table>
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  V.I. Arnol'd,  "Mathematical methods of classical mechanics" , Springer  (1978)  (Translated from Russian)</TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top">  E.T. Whittaker,  "Analytical dynamics of particles and rigid bodies" , Dover, reprint  (1944)</TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top">  F.R. [F.R. Gantmakher] Gantmacher,  "Lectures in analytical mechanics" , MIR  (1975)  (Translated from Russian)</TD></TR><TR><TD valign="top">[a4]</TD> <TD valign="top">  J.L. Lagrange,  "Mécanique analytique" , '''1–2''' , Blanchard, reprint , Paris  (1965)  ((Also: Oeuvres, Vol. 11.))</TD></TR></table>

Latest revision as of 22:15, 5 June 2020


principle of stationary action

A variational integral principle in the dynamics of holonomic systems restricted by ideal stationary constraints and occurring under the action of potential forces that do not explicitly depend on time.

According to Lagrange's principle, in a real motion of a holonomic system for which the energy integral $ T + V = h $ exists, between a certain initial position $ A _ {0} $ and a final position $ A _ {1} $, the Lagrange action

$$ \int\limits _ {t _ {0} } ^ { t } 2 T dt = \int\limits _ {A _ {0} } ^ { {A } _ {1} } \sum _ \nu m _ \nu v _ \nu \cdot d r _ \nu $$

has a stationary value in comparison with the kinematically possible motions between these positions with the same energy $ h $ as in the real motion. Here $ T $ and $ V $ are the kinetic and the potential energy of the system, $ m _ \nu v _ \nu $ is the amount of motion (momentum) of the $ \nu $- th point of the system and $ t _ {0} $ and $ t $ are the instants when the system passes through the positions $ A _ {0} $ and $ A _ {1} $.

If the initial and final positions of the system are sufficiently close to one another, then the Lagrange action has a minimum for a real motion; in this connection the Lagrange principle is also called the principle of least action in Lagrange's form.

The Lagrange principle reduces the problem of determining a real motion of the system to the variational Lagrange problem; it expresses a condition that is necessary and sufficient for a real motion [4].

The Lagrange principle in implicit form was first stated by P.L.M. Maupertuis [1]; L. Euler [2] gave a proof of it for the case of the motion of one material point in a central field. J.L. Lagrange [3] extended this principle to more general problems.

References

[1] P.L.M. Maupertuis, Histoire l'Acad. Royale Sci. Paris 1744 (1748) pp. 417
[2] L. Euler, "Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes sive solutio problematis isoperimetrici latissimo sensu accepti" , Lausanne-Geneva (1744)
[3] J.L. Lagrange, "Essai d'une nouvelle méthode pour déterminer les maxima et les minima des formules intégrales indéfinies" J.A. Serret (ed.) , Oeuvres , 1 , G. Olms, reprint (1973) pp. 333–362
[4] G.K. Suslov, "Theoretical mechanics" , Moscow (1944) (In Russian)

Comments

References

[a1] V.I. Arnol'd, "Mathematical methods of classical mechanics" , Springer (1978) (Translated from Russian)
[a2] E.T. Whittaker, "Analytical dynamics of particles and rigid bodies" , Dover, reprint (1944)
[a3] F.R. [F.R. Gantmakher] Gantmacher, "Lectures in analytical mechanics" , MIR (1975) (Translated from Russian)
[a4] J.L. Lagrange, "Mécanique analytique" , 1–2 , Blanchard, reprint , Paris (1965) ((Also: Oeuvres, Vol. 11.))
How to Cite This Entry:
Lagrange principle. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Lagrange_principle&oldid=47558
This article was adapted from an original article by V.V. Rumyantsev (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article