International Journal of Theoretical and Mathematical Physics
p-ISSN: 2167-6844 e-ISSN: 2167-6852
2019; 9(5): 136-152
doi:10.5923/j.ijtmp.20190905.03

Vasil Angelov
Department of of Mathematics, University of Mining and Geology “St. I. Rilski”, Sofia, Bulgaria
Correspondence to: Vasil Angelov, Department of of Mathematics, University of Mining and Geology “St. I. Rilski”, Sofia, Bulgaria.
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Copyright © 2019 The Author(s). Published by Scientific & Academic Publishing.
This work is licensed under the Creative Commons Attribution International License (CC BY).
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In a previous paper we have derived a new form of the radiation term without changing the Dirac physical assumptions. We have showed also that the fourth Dirac equation is a consequence of the first three ones, that implies the Dirac system is not overdetermined – three equations for three unknown functions. Here we replace the Dirac local expansions with nonlocal formulation of the problem. So we have obtained a system of first order neutral differential equations with respect to the unknown velocities containing both retarded and advanced arguments. Since the accelerator theory relies on the Dirac-Lorentz equation the obtained periodic solutions can be applied directly to the study of betatron equation.
Keywords: Dirac-Lorentz equation, Fixed point method, Periodic operator, Periodic solution
Cite this paper: Vasil Angelov, Periodic Solutions of the Dirac-Lorentz Equation, International Journal of Theoretical and Mathematical Physics, Vol. 9 No. 5, 2019, pp. 136-152. doi: 10.5923/j.ijtmp.20190905.03.
![]() | (1) |
are the coordinates of the electron, e is its charge, m – its rest mass, c – the speed of the light, the dot is a differentiation with respect to the arc length, i.e.
, and the Einstein summation convention is valid. The second term in (1) is the Abraham four-vector of radiation reaction derived also by Dirac [3]. Here we replace the radiation term in (1) by the one obtained in [1]. We consider just first three equations because in [1] is proved that the fourth one is a consequence of the rest ones. We have applied a similar form of the radiation terms to two-body problem of classical electrodynamics [4]- [6]. Many results concerning radiation terms are contained in [7]-[32]. They are based on various methods. Here we use the fixed point method from [33]. The derivation of the new form of the radiation term is based on the relativistic form of the retarded and advanced Lienard-Wiechert potentials [8]-[10], [34], [35]. We stand on the theory of differential equations of neutral type with both retarded and advanced arguments caused by the finite propagation of the interaction – the basic assumption of the Einstein relativistic theory. So Dirac equations become second order neutral equations. The main goal of the present paper is to prove an existence-uniqueness of a periodic solution for Dirac equations. We use an operator formulation of the periodic problem from [36]. In view of [37]-[39] we are able to apply the results obtained to betatron radiation.The paper consists of six sections. In Section 2 we derive the Dirac equations using retarded and advanced potentials. In Section 3 we derive a new form of the radiation term. In Section 4 we formulate a periodic problem and give some preliminary assertions. In Section 5 we give an operator formulation of the periodic problem and by a suitable fixed point theorem prove an existence-uniqueness of periodic solution for Dirac equations. Section 6 contains a conclusion remark.
be any event. The unit tangent vector to L at A is
where
and
is the scalar product in 4-dimensional Minkowski space, while
is the scalar product in 3-dimensional Euclidian subspace.Let
be the intersection of L with the null-cone drawn into the past from A, and let
be the intersection of L with the null-cone drawn into the future from A where
and
Let
be the unit tangent vector to the world line L at
, where
and let
be the unit tangent vector to L at
, where
Let
be the retarded isotropic vector
and let
be the advanced isotropic vector
In accordance with the Dirac assumptions [3] the radiation term is defined as a half of the difference between both retarded and advanced potentials, that is,
where
are the Lienard-Wiechert retarded and advanced potentials (cf. [8]-[10], [34], [35]).So that the Dirac physical assumptions lead to the following form of the equations of motion:
or
Further on we assume (cf. [1]) that(AR):
In fact, postulating (AR) we extend the relation between the relativistic and Newton absolute time. Since
and
lie on the trajectory L we obtain
and
where 
where
Therefore the isotropic vectors become
and
In general case the functions
can be obtained as solutions of the functional equations
or
In what follows we briefly repeat the calculations from [1]:![]() | (2) |
Here
and
is the electric field intensity vector, and
− the magnetic field intensity vector.
Differentiating the relation
with respect to
, considering
we obtain
In a similar way differentiating
with respect to
(considering
) we obtain
We derive the radiation term under the Dirac assumptions (D):
where
is a small parameter.The Dirac assumption is justified by the fact that, for example, the electron radiation time is
sec.Applying the Taylor theorem under assumption (D) we get
It follows
. Consequently
and then
Therefore the above system becomes![]() | (3) |
we obtain
Denoting by
we write the system
in the form![]() | (4) |
. Assumption (C):
for some constant
.Therefore
and the determinant of the above system is obviously different from zero
Consequently, the uni- que solution of (4) is![]() | (5) |
we get![]() | (6) |
- periodic solution
of the system (6) on the interval
with initial conditions
,
and
where
are prescribed
-periodic initial functions.Let
be the set of all
-periodic functions from
whose derivatives of arbitrary order belong to
. The functions from
are considered as all infinite differentiable functions on
having continuous extensions on
. Introduce the function sets:
where
,
Remark 1. It is easy to verify that substituting
we get
We define the following family of pseudo-metrics
Since for
we have
It follows
and then we put
Further on we set
Lemma 1. If
then
is
-periodic function.Proof: Let us set
and then we obtain
. Therefore
Lemma 1 is thus proved.Define the operator
where by assumption
and
are the right-hand sides of (6).Lemma 2. ([36]) For every
it follows
Assumptions (H-E): The functions 
are
-periodic and smooth in t and 
Lemma 3. (Main Lemma) The periodic problem (6) has a solution
iff the operator B has a fixed point belonging to
, provided
where
are positive constants.Proof: Let
be a
-periodic solution of the system
. Then after integration in view of
(that is
and
) we obtain![]() | (7) |
Besides in view of (7) we have
that implies
Consequently,
can be written in the form
The last equalities mean that B has a fixed point in
.Conversely, let
be a fixed point of B. Then the last equalities are satisfied and substituting
we get
that implies
We show that
. Indeed, Let us suppose that
. Then we obtain
which implies
since
In a similar way we get
Consequently
Since
= const for sufficiently large
and small
we can obtain
. Therefore
becomes
Differentiating the last equality we obtain the required assertion.Lemma 3 is thus proved.
are defined on
and are such that their translations to the right on
coincide with some functions from
and
, where
for some positive integer m.2. The components of intensity electric and magnetic vectors satisfy the assumptions (H-E); 3. The following inequalities are satisfied:
Then there is a unique
-periodic solution of (6)
.Proof: In view of the Main Lemma 3 we have to prove that the operator B possesses a unique fixed point. This fixed point is a
-periodic solution of (6). The set
turns out into a uniform space with a saturated family of pseudo-metrics for
:
since
where the index set is
Define the operator
by the formulas
, where
are the right-hand sides of (6).We show that B maps
into itself. Since
we have shown in the Main Lemma 3 that
Therefore
First we check the following equality
Further on for
we obtain
We have
Therefore
Finally we reach the estimate
Let us estimate the derivatives
Then in view of
we obtain
we obtain
But
and consequently
and so on. Therefore
.Remark 2. In order to obtain suitable estimations for higher derivatives we use the chain of inequalities
In this way we compensate the degree of
in the nominator by the degree of
in the denominator.In what follows we show that B is contractive operator.First we notice that the following Lipschitz estimate for the expression
is valid:
and in a similar way from
we obtain
Then


For the second term we obtain
For the third term we get
Therefore
Consequently
In what follows we make the same estimates for the derivatives of the operator functions B (for higher derivatives we recall Remark1). Indeed,
and

Therefore the operator B is contractive in the sense of [35]. Its fixed point in view of the Main lemma is a
periodic solution of (6).Theorem 1 is thus proved.