Difference between revisions of "Poincaré equations"
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General equations of the mechanics of holonomic systems (cf. [[Holonomic system|Holonomic system]]) presented with the help of a certain Lie algebra of infinitesimal transformations. | General equations of the mechanics of holonomic systems (cf. [[Holonomic system|Holonomic system]]) presented with the help of a certain Lie algebra of infinitesimal transformations. | ||
− | Let | + | Let $ x _ {i} $, |
+ | $ i = 1 \dots n $, | ||
+ | be variables determining the position of a holonomic mechanical system constrained by ideal constraints depending explicitly on time. If the system has $ k $ | ||
+ | degrees of freedom, then there is an intransitive algebra of infinitesimal transformations | ||
+ | |||
+ | $$ | ||
+ | X _ {0} = | ||
+ | \frac \partial {\partial t } | ||
+ | |||
+ | + \sum _{j=1}^ { n } | ||
+ | \xi _ {0} ^ {j} | ||
+ | \frac \partial {\partial x _ {j} } | ||
+ | ,\ \ | ||
+ | X _ {a} = \sum _ {j=1}^ { n } \xi _ \alpha ^ {j} | ||
− | + | \frac \partial {\partial x _ {j} } | |
+ | , | ||
+ | $$ | ||
− | + | $$ | |
+ | \alpha = 1 \dots k , | ||
+ | $$ | ||
− | enabling the system to be carried at the moment of time | + | enabling the system to be carried at the moment of time $ t $ |
+ | from the position $ x _ {i} $ | ||
+ | to the infinitesimally-near actual position $ x _ {i} + d x _ {i} $ | ||
+ | and the virtual position $ x _ {i} + \delta x _ {i} $ | ||
+ | by infinitesimal transformations $ ( X _ {0} + \sum _ {\alpha = 1 } ^ {k} \eta _ \alpha X _ \alpha ) d t $ | ||
+ | of the algebra and $ \sum _ {\alpha = 1 } ^ {k} \omega _ {i} X _ {i} $ | ||
+ | of the subalgebra, respectively. Here $ \omega _ \alpha $ | ||
+ | and $ \eta _ \alpha $, | ||
+ | the independent variables determining the virtual and actual displacements respectively, are connected by the equations | ||
− | + | $$ | |
+ | \delta {\eta _ {i} } = \ | ||
− | + | \frac{d \omega _ {i} }{dt} | |
+ | - | ||
+ | \sum _ {\alpha , \beta = 1 } ^ { k } c _ {\alpha \beta i } \omega _ \alpha \eta _ \beta ,\ \ | ||
+ | i = 1 \dots k , | ||
+ | $$ | ||
− | + | if the algebra of virtual displacements $ X _ \alpha $ | |
+ | is determined by its structure constants $ c _ {\alpha \beta i } $: | ||
− | + | $$ | |
+ | ( X _ \alpha X _ \beta ) = \ | ||
+ | X _ \alpha X _ \beta - X _ \beta X _ \alpha = \ | ||
+ | \sum _ {i=1}^ { k } c _ {\alpha \beta i } X _ {i} , | ||
+ | $$ | ||
− | + | $$ | |
+ | \alpha , \beta = 1 \dots k , | ||
+ | $$ | ||
− | + | and the operator $ X _ {0} $ | |
+ | commutes with the algebra of virtual displacements | ||
+ | |||
+ | $$ | ||
+ | ( X _ {0} X _ \alpha ) = 0 ,\ \alpha = 1 \dots k . | ||
+ | $$ | ||
Below these conditions are assumed to hold. | Below these conditions are assumed to hold. | ||
− | The Poincaré equations are ordinary first-order (with respect to | + | The Poincaré equations are ordinary first-order (with respect to $ \eta _ {j} $) |
+ | differential equations | ||
− | + | $$ \tag{1 } | |
− | + | \frac{d}{dt} | |
− | + | \frac{\partial L }{\partial \eta _ {j} } | |
+ | \ | ||
+ | = \sum _ {\alpha , \beta = 1 } ^ { k } c _ {\alpha j \beta } | ||
+ | \eta _ \alpha | ||
+ | \frac{\partial L }{\partial \eta _ \beta } | ||
− | is the Lagrange function, | + | + X _ {j} L , |
+ | $$ | ||
+ | |||
+ | where $ j = 1 \dots k $, | ||
+ | |||
+ | $$ | ||
+ | L ( t , x _ {1} \dots x _ {n} , \eta _ {1} \dots \eta _ {k} ) = \ | ||
+ | T + U | ||
+ | $$ | ||
+ | |||
+ | is the Lagrange function, $ T ( t , x , \eta ) $ | ||
+ | is the kinetic energy and $ U ( t , x ) $ | ||
+ | is the force function. | ||
The equations (1) were first obtained by H. Poincaré (see [[#References|[1]]]) in the case when the algebra of virtual displacements is transitive and the constraints do not depend explicitly on time, and he applied them (see [[#References|[2]]]) to investigate the motion of a solid body with an ellipsoidal cavity, entirely filled by a uniformly vortex moving ideal fluid. N.G. Chetaev (see [[#References|[3]]]) generalized and developed the theory of the Poincaré equations to the case where the algebra of displacements is intransitive and the constraints depend explicitly on time (see [[#References|[3]]]–[[#References|[5]]]) and also converted them to a simpler canonical form (see [[Chetaev equations|Chetaev equations]]). In particular, he gave (see [[#References|[5]]]) a method for constructing the algebra of virtual and actual displacements when the holonomic constraints are given by a differential form and he introduced the important concept of cyclic displacements. | The equations (1) were first obtained by H. Poincaré (see [[#References|[1]]]) in the case when the algebra of virtual displacements is transitive and the constraints do not depend explicitly on time, and he applied them (see [[#References|[2]]]) to investigate the motion of a solid body with an ellipsoidal cavity, entirely filled by a uniformly vortex moving ideal fluid. N.G. Chetaev (see [[#References|[3]]]) generalized and developed the theory of the Poincaré equations to the case where the algebra of displacements is intransitive and the constraints depend explicitly on time (see [[#References|[3]]]–[[#References|[5]]]) and also converted them to a simpler canonical form (see [[Chetaev equations|Chetaev equations]]). In particular, he gave (see [[#References|[5]]]) a method for constructing the algebra of virtual and actual displacements when the holonomic constraints are given by a differential form and he introduced the important concept of cyclic displacements. | ||
− | Displacements | + | Displacements $ X _ {r} $, |
+ | $ r = s + 1 \dots k $, | ||
+ | are said to be cyclic if they satisfy the conditions: 1) $ X _ {r} L = 0 $; | ||
+ | 2) $ ( X _ {r} X _ \beta ) = 0 $, | ||
+ | $ r = s + 1 \dots k $, | ||
+ | $ \beta = 1 \dots k $. | ||
− | According to 2) the cyclic displacements | + | According to 2) the cyclic displacements $ X _ {r} $ |
+ | form an Abelian subalgebra of the algebra of virtual displacements which commutes with all the operators $ X _ \beta $. | ||
+ | For cyclic displacements the first integrals of the Poincaré equations, | ||
− | + | $$ | |
− | + | \frac{\partial L }{\partial \eta _ {r} } | |
+ | \ | ||
+ | = a _ {r} = \textrm{ const } ,\ \ | ||
+ | r = s + 1 \dots k , | ||
+ | $$ | ||
− | + | exist. From these relations the variables $ \eta _ {r} $ | |
+ | can be expressed in terms of the constants $ a _ {r} $ | ||
+ | and the variables $ t $, | ||
+ | $ x _ {i} $, | ||
+ | $ \eta _ {1} \dots \eta _ {s} $, | ||
+ | and one can introduce the Routh function | ||
− | + | $$ | |
+ | R ( t , x _ {1} \dots x _ {n} ; \eta _ {1} \dots \eta _ {s} ; \ | ||
+ | a _ {s+} 1 \dots a _ {k} ) = | ||
+ | $$ | ||
+ | |||
+ | $$ | ||
+ | = \ | ||
+ | L - \sum _ {r = s + 1 } ^ { k } | ||
+ | \frac{\partial L }{\partial \eta _ {r} } | ||
+ | \eta _ {r} . | ||
+ | $$ | ||
Then for the non-cyclic displacements the Poincaré equations take the form | Then for the non-cyclic displacements the Poincaré equations take the form | ||
− | + | $$ \tag{2 } | |
+ | |||
+ | \frac{d}{dt} | ||
+ | |||
+ | \frac{\partial R }{\partial \eta _ {j} } | ||
+ | \ | ||
+ | = \sum c _ {\alpha j \beta } \eta _ \alpha | ||
+ | \frac{\partial R }{\partial \eta _ \beta } | ||
+ | + | ||
+ | \sum c _ {\alpha j \gamma } \eta _ \alpha a _ \gamma + X _ {j} R , | ||
+ | $$ | ||
+ | |||
+ | $$ | ||
+ | \alpha , j , \beta = 1 \dots s ; \ \gamma = s + 1 \dots k . | ||
+ | $$ | ||
− | + | After integrating the equations (2) the values $ \eta _ {r} $ | |
+ | are determined by the equations | ||
− | + | $$ | |
+ | \eta _ {r} = - | ||
− | + | \frac{\partial R }{\partial a _ {r} } | |
+ | ,\ \ | ||
+ | r = s + 1 \dots k . | ||
+ | $$ | ||
− | If, in addition, | + | If, in addition, $ c _ {\alpha j \gamma } = 0 $, |
+ | $ \alpha , j = 1 \dots s $, | ||
+ | $ \gamma = s + 1 \dots k $, | ||
+ | that is, if the non-cyclic displacements $ X _ \beta $, | ||
+ | $ \beta = 1 \dots k $, | ||
+ | form a subalgebra of the algebra of virtual displacements, then the mechanical system corresponding to this subalgebra forms some sort of independent holonomic system with $ s $ | ||
+ | degrees of freedom, described by the equations (1) when $ \alpha , j , \beta = 1 \dots s $, | ||
+ | where the role of the function $ L $ | ||
+ | is played by the function $ R $. | ||
− | The Poincaré equations contain as particular cases: the [[Lagrange equations (in mechanics)|Lagrange equations (in mechanics)]] when the transformation algebra of infinitesimal increments in one of the variables reduces to a commutative algebra of transformations; and the [[Euler equation|Euler equation]] for the rotation of a solid body, when the | + | The Poincaré equations contain as particular cases: the [[Lagrange equations (in mechanics)|Lagrange equations (in mechanics)]] when the transformation algebra of infinitesimal increments in one of the variables reduces to a commutative algebra of transformations; and the [[Euler equation|Euler equation]] for the rotation of a solid body, when the $ \eta _ {i} $ |
+ | are taken to be the projections $ p $, | ||
+ | $ q $ | ||
+ | and $ r $ | ||
+ | of the instantaneous angular velocity. | ||
====References==== | ====References==== | ||
<table><TR><TD valign="top">[1]</TD> <TD valign="top"> H. Poincaré, ''C.R. Acad. Sci. Paris'' , '''132''' (1901) pp. 369–371</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top"> H. Poincaré, ''Bull. Astron.'' , '''27''' (1910) pp. 321–356</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top"> N.G. Chetaev, ''Dokl. Akad. Nauk SSSR'' , '''7''' (1928) pp. 103–104</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top"> N.G. Chetaev, "Sur les équations de Poincaré" ''C.R. Acad. Sci. Paris'' , '''185''' (1927) pp. 1577–1578</TD></TR><TR><TD valign="top">[5]</TD> <TD valign="top"> N.G. Chetaev, ''Prikl. Mat. i. Mekh.'' , '''5''' : 2 (1941) pp. 253–262</TD></TR></table> | <table><TR><TD valign="top">[1]</TD> <TD valign="top"> H. Poincaré, ''C.R. Acad. Sci. Paris'' , '''132''' (1901) pp. 369–371</TD></TR><TR><TD valign="top">[2]</TD> <TD valign="top"> H. Poincaré, ''Bull. Astron.'' , '''27''' (1910) pp. 321–356</TD></TR><TR><TD valign="top">[3]</TD> <TD valign="top"> N.G. Chetaev, ''Dokl. Akad. Nauk SSSR'' , '''7''' (1928) pp. 103–104</TD></TR><TR><TD valign="top">[4]</TD> <TD valign="top"> N.G. Chetaev, "Sur les équations de Poincaré" ''C.R. Acad. Sci. Paris'' , '''185''' (1927) pp. 1577–1578</TD></TR><TR><TD valign="top">[5]</TD> <TD valign="top"> N.G. Chetaev, ''Prikl. Mat. i. Mekh.'' , '''5''' : 2 (1941) pp. 253–262</TD></TR></table> |
Latest revision as of 20:21, 17 January 2024
General equations of the mechanics of holonomic systems (cf. Holonomic system) presented with the help of a certain Lie algebra of infinitesimal transformations.
Let $ x _ {i} $, $ i = 1 \dots n $, be variables determining the position of a holonomic mechanical system constrained by ideal constraints depending explicitly on time. If the system has $ k $ degrees of freedom, then there is an intransitive algebra of infinitesimal transformations
$$ X _ {0} = \frac \partial {\partial t } + \sum _{j=1}^ { n } \xi _ {0} ^ {j} \frac \partial {\partial x _ {j} } ,\ \ X _ {a} = \sum _ {j=1}^ { n } \xi _ \alpha ^ {j} \frac \partial {\partial x _ {j} } , $$
$$ \alpha = 1 \dots k , $$
enabling the system to be carried at the moment of time $ t $ from the position $ x _ {i} $ to the infinitesimally-near actual position $ x _ {i} + d x _ {i} $ and the virtual position $ x _ {i} + \delta x _ {i} $ by infinitesimal transformations $ ( X _ {0} + \sum _ {\alpha = 1 } ^ {k} \eta _ \alpha X _ \alpha ) d t $ of the algebra and $ \sum _ {\alpha = 1 } ^ {k} \omega _ {i} X _ {i} $ of the subalgebra, respectively. Here $ \omega _ \alpha $ and $ \eta _ \alpha $, the independent variables determining the virtual and actual displacements respectively, are connected by the equations
$$ \delta {\eta _ {i} } = \ \frac{d \omega _ {i} }{dt} - \sum _ {\alpha , \beta = 1 } ^ { k } c _ {\alpha \beta i } \omega _ \alpha \eta _ \beta ,\ \ i = 1 \dots k , $$
if the algebra of virtual displacements $ X _ \alpha $ is determined by its structure constants $ c _ {\alpha \beta i } $:
$$ ( X _ \alpha X _ \beta ) = \ X _ \alpha X _ \beta - X _ \beta X _ \alpha = \ \sum _ {i=1}^ { k } c _ {\alpha \beta i } X _ {i} , $$
$$ \alpha , \beta = 1 \dots k , $$
and the operator $ X _ {0} $ commutes with the algebra of virtual displacements
$$ ( X _ {0} X _ \alpha ) = 0 ,\ \alpha = 1 \dots k . $$
Below these conditions are assumed to hold.
The Poincaré equations are ordinary first-order (with respect to $ \eta _ {j} $) differential equations
$$ \tag{1 } \frac{d}{dt} \frac{\partial L }{\partial \eta _ {j} } \ = \sum _ {\alpha , \beta = 1 } ^ { k } c _ {\alpha j \beta } \eta _ \alpha \frac{\partial L }{\partial \eta _ \beta } + X _ {j} L , $$
where $ j = 1 \dots k $,
$$ L ( t , x _ {1} \dots x _ {n} , \eta _ {1} \dots \eta _ {k} ) = \ T + U $$
is the Lagrange function, $ T ( t , x , \eta ) $ is the kinetic energy and $ U ( t , x ) $ is the force function.
The equations (1) were first obtained by H. Poincaré (see [1]) in the case when the algebra of virtual displacements is transitive and the constraints do not depend explicitly on time, and he applied them (see [2]) to investigate the motion of a solid body with an ellipsoidal cavity, entirely filled by a uniformly vortex moving ideal fluid. N.G. Chetaev (see [3]) generalized and developed the theory of the Poincaré equations to the case where the algebra of displacements is intransitive and the constraints depend explicitly on time (see [3]–[5]) and also converted them to a simpler canonical form (see Chetaev equations). In particular, he gave (see [5]) a method for constructing the algebra of virtual and actual displacements when the holonomic constraints are given by a differential form and he introduced the important concept of cyclic displacements.
Displacements $ X _ {r} $, $ r = s + 1 \dots k $, are said to be cyclic if they satisfy the conditions: 1) $ X _ {r} L = 0 $; 2) $ ( X _ {r} X _ \beta ) = 0 $, $ r = s + 1 \dots k $, $ \beta = 1 \dots k $.
According to 2) the cyclic displacements $ X _ {r} $ form an Abelian subalgebra of the algebra of virtual displacements which commutes with all the operators $ X _ \beta $. For cyclic displacements the first integrals of the Poincaré equations,
$$ \frac{\partial L }{\partial \eta _ {r} } \ = a _ {r} = \textrm{ const } ,\ \ r = s + 1 \dots k , $$
exist. From these relations the variables $ \eta _ {r} $ can be expressed in terms of the constants $ a _ {r} $ and the variables $ t $, $ x _ {i} $, $ \eta _ {1} \dots \eta _ {s} $, and one can introduce the Routh function
$$ R ( t , x _ {1} \dots x _ {n} ; \eta _ {1} \dots \eta _ {s} ; \ a _ {s+} 1 \dots a _ {k} ) = $$
$$ = \ L - \sum _ {r = s + 1 } ^ { k } \frac{\partial L }{\partial \eta _ {r} } \eta _ {r} . $$
Then for the non-cyclic displacements the Poincaré equations take the form
$$ \tag{2 } \frac{d}{dt} \frac{\partial R }{\partial \eta _ {j} } \ = \sum c _ {\alpha j \beta } \eta _ \alpha \frac{\partial R }{\partial \eta _ \beta } + \sum c _ {\alpha j \gamma } \eta _ \alpha a _ \gamma + X _ {j} R , $$
$$ \alpha , j , \beta = 1 \dots s ; \ \gamma = s + 1 \dots k . $$
After integrating the equations (2) the values $ \eta _ {r} $ are determined by the equations
$$ \eta _ {r} = - \frac{\partial R }{\partial a _ {r} } ,\ \ r = s + 1 \dots k . $$
If, in addition, $ c _ {\alpha j \gamma } = 0 $, $ \alpha , j = 1 \dots s $, $ \gamma = s + 1 \dots k $, that is, if the non-cyclic displacements $ X _ \beta $, $ \beta = 1 \dots k $, form a subalgebra of the algebra of virtual displacements, then the mechanical system corresponding to this subalgebra forms some sort of independent holonomic system with $ s $ degrees of freedom, described by the equations (1) when $ \alpha , j , \beta = 1 \dots s $, where the role of the function $ L $ is played by the function $ R $.
The Poincaré equations contain as particular cases: the Lagrange equations (in mechanics) when the transformation algebra of infinitesimal increments in one of the variables reduces to a commutative algebra of transformations; and the Euler equation for the rotation of a solid body, when the $ \eta _ {i} $ are taken to be the projections $ p $, $ q $ and $ r $ of the instantaneous angular velocity.
References
[1] | H. Poincaré, C.R. Acad. Sci. Paris , 132 (1901) pp. 369–371 |
[2] | H. Poincaré, Bull. Astron. , 27 (1910) pp. 321–356 |
[3] | N.G. Chetaev, Dokl. Akad. Nauk SSSR , 7 (1928) pp. 103–104 |
[4] | N.G. Chetaev, "Sur les équations de Poincaré" C.R. Acad. Sci. Paris , 185 (1927) pp. 1577–1578 |
[5] | N.G. Chetaev, Prikl. Mat. i. Mekh. , 5 : 2 (1941) pp. 253–262 |
Poincaré equations. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Poincar%C3%A9_equations&oldid=22925