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A branch of [[Relativity theory|relativity theory]] devoted to the study of the movement of material bodies under the action of forces applied to them.
 
A branch of [[Relativity theory|relativity theory]] devoted to the study of the movement of material bodies under the action of forces applied to them.
  
 
In relativity theory free material points, i.e. points not subject to the action of forces, have as their world lines time-like geodesics or isotropic geodesics. This fact is an expression of the [[Law of inertia|law of inertia]] in relativity theory.
 
In relativity theory free material points, i.e. points not subject to the action of forces, have as their world lines time-like geodesics or isotropic geodesics. This fact is an expression of the [[Law of inertia|law of inertia]] in relativity theory.
  
If there are forces acting on a particle, then its world line does not coincide with a geodesic. The movement of a particle is described with reference to the concepts of a four-dimensional energy-momentum vector <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810801.png" />, and the four-dimensional force vector <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810802.png" />. Thus,
+
If there are forces acting on a particle, then its world line does not coincide with a geodesic. The movement of a particle is described with reference to the concepts of a four-dimensional energy-momentum vector $  p  ^ {i} $,  
 +
and the four-dimensional force vector $  g  ^ {i} $.  
 +
Thus,
 +
 
 +
$$ \tag{1 }
 +
p  ^ {i}  =  \left (
 +
\frac{\mathbf E }{c}
 +
;  \mathbf p \right ) ,
 +
$$
  
<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/r/r081/r081080/r0810803.png" /></td> <td valign="top" style="width:5%;text-align:right;">(1)</td></tr></table>
+
where  $  \mathbf E $
 +
is the energy of the particle,  $  m $
 +
is its rest mass and  $  \mathbf p $
 +
is its three-dimensional momentum. The vector  $  g  ^ {i} $
 +
is defined by the relation
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810804.png" /> is the energy of the particle, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810805.png" /> is its rest mass and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810806.png" /> is its three-dimensional momentum. The vector <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810807.png" /> is defined by the relation
+
$$
 +
g  ^ {i}  = \left ( {\mathbf F } \cdot
 +
\frac{\mathbf V }{c  ^ {2} \sqrt {1 - V  ^ {2} /c  ^ {2} } }
  
<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/r/r081/r081080/r0810808.png" /></td> </tr></table>
+
;
 +
\frac{\mathbf F }{c \sqrt {1 - V  ^ {2} /c  ^ {2} } }
 +
\right ) ,
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r0810809.png" /> is a three-dimensional force and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r08108010.png" /> is the velocity. By using these vectors, the basic equations of relativistic dynamics can be written in a form similar to that of the equations of Newton's second law:
+
where $  \mathbf F $
 +
is a three-dimensional force and $  \mathbf V $
 +
is the velocity. By using these vectors, the basic equations of relativistic dynamics can be written in a form similar to that of the equations of Newton's second law:
  
<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/r/r081/r081080/r08108011.png" /></td> <td valign="top" style="width:5%;text-align:right;">(2)</td></tr></table>
+
$$ \tag{2 }
 +
g  ^ {i}  =
 +
\frac{dp  ^ {i} }{ds}
 +
  = mc
 +
\frac{du  ^ {i} }{ds}
 +
.
 +
$$
  
The concrete form of the force <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r08108012.png" /> is determined in those branches of the theory of relativity that examine the concrete properties of various interactions. For example, the force acting on a particle in an electromagnetic field — the Lorentz force — takes the form
+
The concrete form of the force $  g  ^ {i} $
 +
is determined in those branches of the theory of relativity that examine the concrete properties of various interactions. For example, the force acting on a particle in an electromagnetic field — the Lorentz force — takes the form
  
<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/r/r081/r081080/r08108013.png" /></td> </tr></table>
+
$$
 +
g  ^ {i}  =
 +
\frac{e}{c}
 +
F ^ { ik } u _ {k} ,
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r08108014.png" /> is the charge of the particle, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r08108015.png" /> is the tensor of the electromagnetic field and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/r/r081/r081080/r08108016.png" /> is the four-dimensional velocity.
+
where $  e $
 +
is the charge of the particle, $  F ^ { ik } $
 +
is the tensor of the electromagnetic field and $  u _ {k} $
 +
is the four-dimensional velocity.
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  L.D. Landau,  E.M. Lifshitz,  "The theory of fields" , Pergamon  (1965)  (Translated from Russian)</TD></TR></table>
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  L.D. Landau,  E.M. Lifshitz,  "The theory of fields" , Pergamon  (1965)  (Translated from Russian)</TD></TR></table>
 
 
  
 
====Comments====
 
====Comments====
 
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  W. Rindler,  "Essential relativity" , Springer  (1977)</TD></TR></table>
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  W. Rindler,  "Essential relativity" , Springer  (1977)</TD></TR></table>

Latest revision as of 08:10, 6 June 2020


A branch of relativity theory devoted to the study of the movement of material bodies under the action of forces applied to them.

In relativity theory free material points, i.e. points not subject to the action of forces, have as their world lines time-like geodesics or isotropic geodesics. This fact is an expression of the law of inertia in relativity theory.

If there are forces acting on a particle, then its world line does not coincide with a geodesic. The movement of a particle is described with reference to the concepts of a four-dimensional energy-momentum vector $ p ^ {i} $, and the four-dimensional force vector $ g ^ {i} $. Thus,

$$ \tag{1 } p ^ {i} = \left ( \frac{\mathbf E }{c} ; \mathbf p \right ) , $$

where $ \mathbf E $ is the energy of the particle, $ m $ is its rest mass and $ \mathbf p $ is its three-dimensional momentum. The vector $ g ^ {i} $ is defined by the relation

$$ g ^ {i} = \left ( {\mathbf F } \cdot \frac{\mathbf V }{c ^ {2} \sqrt {1 - V ^ {2} /c ^ {2} } } ; \frac{\mathbf F }{c \sqrt {1 - V ^ {2} /c ^ {2} } } \right ) , $$

where $ \mathbf F $ is a three-dimensional force and $ \mathbf V $ is the velocity. By using these vectors, the basic equations of relativistic dynamics can be written in a form similar to that of the equations of Newton's second law:

$$ \tag{2 } g ^ {i} = \frac{dp ^ {i} }{ds} = mc \frac{du ^ {i} }{ds} . $$

The concrete form of the force $ g ^ {i} $ is determined in those branches of the theory of relativity that examine the concrete properties of various interactions. For example, the force acting on a particle in an electromagnetic field — the Lorentz force — takes the form

$$ g ^ {i} = \frac{e}{c} F ^ { ik } u _ {k} , $$

where $ e $ is the charge of the particle, $ F ^ { ik } $ is the tensor of the electromagnetic field and $ u _ {k} $ is the four-dimensional velocity.

References

[1] L.D. Landau, E.M. Lifshitz, "The theory of fields" , Pergamon (1965) (Translated from Russian)

Comments

References

[a1] W. Rindler, "Essential relativity" , Springer (1977)
How to Cite This Entry:
Relativistic dynamics. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Relativistic_dynamics&oldid=48499
This article was adapted from an original article by D.D. Sokolov (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article