• Source: Newtonian dynamics

In physics, Newtonian dynamics (also known as Newtonian mechanics) is the study of the dynamics of a particle or a small body according to Newton's laws of motion.




Mathematical generalizations


Typically, the Newtonian dynamics occurs in a three-dimensional Euclidean space, which is flat. However, in mathematics Newton's laws of motion can be generalized to multidimensional and curved spaces. Often the term Newtonian dynamics is narrowed to Newton's second law




m


a

=

F




{\displaystyle \displaystyle m\,\mathbf {a} =\mathbf {F} }

.




Newton's second law in a multidimensional space


Consider




N



{\displaystyle \displaystyle N}

particles with masses





m

1


,

…
,


m

N





{\displaystyle \displaystyle m_{1},\,\ldots ,\,m_{N}}

in the regular three-dimensional Euclidean space. Let






r


1


,

…
,



r


N





{\displaystyle \displaystyle \mathbf {r} _{1},\,\ldots ,\,\mathbf {r} _{N}}

be their radius-vectors in some inertial coordinate system. Then the motion of these particles is governed by Newton's second law applied to each of them

The three-dimensional radius-vectors






r


1


,

…
,



r


N





{\displaystyle \displaystyle \mathbf {r} _{1},\,\ldots ,\,\mathbf {r} _{N}}

can be built into a single




n
=
3
N



{\displaystyle \displaystyle n=3N}

-dimensional radius-vector. Similarly, three-dimensional velocity vectors






v


1


,

…
,



v


N





{\displaystyle \displaystyle \mathbf {v} _{1},\,\ldots ,\,\mathbf {v} _{N}}

can be built into a single




n
=
3
N



{\displaystyle \displaystyle n=3N}

-dimensional velocity vector:

In terms of the multidimensional vectors (2) the equations (1) are written as

i.e. they take the form of Newton's second law applied to a single particle with the unit mass




m
=
1



{\displaystyle \displaystyle m=1}

.
Definition. The equations (3) are called the
equations of a Newtonian dynamical system in a flat multidimensional Euclidean space, which is called the configuration space of this system. Its points are marked by the radius-vector






r




{\displaystyle \displaystyle \mathbf {r} }

. The space whose points are marked by the pair of vectors




(

r

,

v

)



{\displaystyle \displaystyle (\mathbf {r} ,\mathbf {v} )}

is called the phase space of the dynamical system (3).




Euclidean structure


The configuration space and the phase space of the dynamical system (3) both are Euclidean spaces, i. e. they are equipped with a Euclidean structure. The Euclidean structure of them is defined so that the kinetic energy of the single multidimensional particle with the unit mass




m
=
1



{\displaystyle \displaystyle m=1}

is equal to the sum of kinetic energies of the three-dimensional particles with the masses





m

1


,

…
,


m

N





{\displaystyle \displaystyle m_{1},\,\ldots ,\,m_{N}}

:




Constraints and internal coordinates


In some cases the motion of the particles with the masses





m

1


,

…
,


m

N





{\displaystyle \displaystyle m_{1},\,\ldots ,\,m_{N}}

can be constrained. Typical constraints look like scalar equations of the form

Constraints of the form (5) are called holonomic and scleronomic. In terms of the radius-vector





r




{\displaystyle \displaystyle \mathbf {r} }

of the Newtonian dynamical system (3) they are written as

Each such constraint reduces by one the number of degrees of freedom of the Newtonian dynamical system (3). Therefore, the constrained system has




n
=
3

N
−
K



{\displaystyle \displaystyle n=3\,N-K}

degrees of freedom.
Definition. The constraint equations (6) define an




n



{\displaystyle \displaystyle n}

-dimensional manifold




M



{\displaystyle \displaystyle M}

within the configuration space of the Newtonian dynamical system (3). This manifold




M



{\displaystyle \displaystyle M}

is called the configuration space of the constrained system. Its tangent bundle




T
M



{\displaystyle \displaystyle TM}

is called the phase space of the constrained system.
Let





q

1


,

…
,


q

n





{\displaystyle \displaystyle q^{1},\,\ldots ,\,q^{n}}

be the internal coordinates of a point of




M



{\displaystyle \displaystyle M}

. Their usage is typical for the Lagrangian mechanics. The radius-vector





r




{\displaystyle \displaystyle \mathbf {r} }

is expressed as some definite function of





q

1


,

…
,


q

n





{\displaystyle \displaystyle q^{1},\,\ldots ,\,q^{n}}

:

The vector-function (7) resolves the constraint equations (6) in the sense that upon substituting (7) into (6) the equations (6) are fulfilled identically in





q

1


,

…
,


q

n





{\displaystyle \displaystyle q^{1},\,\ldots ,\,q^{n}}

.




Internal presentation of the velocity vector


The velocity vector of the constrained Newtonian dynamical system is expressed in terms of the partial derivatives of the vector-function
(7):

The quantities








q
˙




1


,

…
,





q
˙




n





{\displaystyle \displaystyle {\dot {q}}^{1},\,\ldots ,\,{\dot {q}}^{n}}

are called internal components of the velocity vector. Sometimes they are denoted with the use of a separate symbol

and then treated as independent variables. The quantities

are used as internal coordinates of a point of the phase space




T
M



{\displaystyle \displaystyle TM}

of the constrained Newtonian dynamical system.




Embedding and the induced Riemannian metric


Geometrically, the vector-function (7) implements an embedding of the configuration space




M



{\displaystyle \displaystyle M}

of the constrained Newtonian dynamical system into the




3

N



{\displaystyle \displaystyle 3\,N}

-dimensional flat configuration space of the unconstrained
Newtonian dynamical system (3). Due to this embedding the Euclidean structure of the ambient space induces the Riemannian metric onto the manifold




M



{\displaystyle \displaystyle M}

. The components of the metric tensor of this induced metric are given by the formula

where




(

,

)



{\displaystyle \displaystyle (\ ,\ )}

is the scalar product associated with the Euclidean structure (4).




Kinetic energy of a constrained Newtonian dynamical system


Since the Euclidean structure of an unconstrained system of




N



{\displaystyle \displaystyle N}

particles is introduced through their kinetic energy, the induced Riemannian structure on the configuration space




N



{\displaystyle \displaystyle N}

of a constrained system preserves this relation to the kinetic energy:

The formula (12) is derived by substituting (8) into (4) and taking into account (11).




Constraint forces


For a constrained Newtonian dynamical system the constraints described by the equations (6) are usually implemented by some mechanical framework. This framework produces some auxiliary forces including the force that maintains the system within its configuration manifold




M



{\displaystyle \displaystyle M}

. Such a maintaining force is perpendicular to




M



{\displaystyle \displaystyle M}

. It is called the normal force. The force





F




{\displaystyle \displaystyle \mathbf {F} }

from (6) is subdivided into two components

The first component in (13) is tangent to the configuration manifold




M



{\displaystyle \displaystyle M}

. The second component is perpendicular to




M



{\displaystyle \displaystyle M}

. In coincides with the normal force





N




{\displaystyle \displaystyle \mathbf {N} }

.
Like the velocity vector (8), the tangent force







F


∥





{\displaystyle \displaystyle \mathbf {F} _{\parallel }}

has its internal presentation

The quantities




F

1


,

…
,


F

n




{\displaystyle F^{1},\,\ldots ,\,F^{n}}

in (14) are called the internal components of the force vector.




Newton's second law in a curved space


The Newtonian dynamical system (3) constrained to the configuration manifold




M



{\displaystyle \displaystyle M}

by the constraint equations (6) is described by the differential equations

where




Γ

i
j


s




{\displaystyle \Gamma _{ij}^{s}}

are Christoffel symbols of the metric connection produced by the Riemannian metric (11).




Relation to Lagrange equations


Mechanical systems with constraints are usually described by Lagrange equations:

where



T
=
T
(

q

1


,
…
,

q

n


,

w

1


,
…
,

w

n


)


{\displaystyle T=T(q^{1},\ldots ,q^{n},w^{1},\ldots ,w^{n})}

is the kinetic energy the constrained dynamical system given by the formula (12). The quantities




Q

1


,

…
,


Q

n




{\displaystyle Q_{1},\,\ldots ,\,Q_{n}}

in
(16) are the inner covariant components of the tangent force vector





F


∥




{\displaystyle \mathbf {F} _{\parallel }}

(see (13) and (14)). They are produced from the inner contravariant components




F

1


,

…
,


F

n




{\displaystyle F^{1},\,\ldots ,\,F^{n}}

of the vector





F


∥




{\displaystyle \mathbf {F} _{\parallel }}

by means of the standard index lowering procedure using the metric (11):

The equations (16) are equivalent to the equations (15). However, the metric (11) and
other geometric features of the configuration manifold




M



{\displaystyle \displaystyle M}

are not explicit in (16). The metric (11) can be recovered from the kinetic energy




T



{\displaystyle \displaystyle T}

by means of the formula




See also


Modified Newtonian dynamics




References

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