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

 

Periodic Solutions of the Dirac-Lorentz Equation

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.

Email:

Copyright © 2019 The Author(s). Published by Scientific & Academic Publishing.

This work is licensed under the Creative Commons Attribution International License (CC BY).
http://creativecommons.org/licenses/by/4.0/

Abstract

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. Introduction

In a previous paper [1] we have derived a general form of the Dirac radiation term [2], [3] based on his original physical assumptions (cf. [3]). In the relativistic case the usually accepted radiation term leads to the well-known Dirac (or Lorentz-Dirac) equations [3]
(1)
where 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.

2. Derivation of Dirac Equations Using Retarded and Advanced Potentials

First we recall some basic notions and denotations following the Synge formalism [35] (cf. also [34]). Consider a charge e describing any curve L in the space-time. Let 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)
(k=1,2,3,4),
where the elements of the electromagnetic tensor are:
Here and is the electric field intensity vector, and − the magnetic field intensity vector.

3. Derivation of the Radiation Term

Following [1] we have to find the relations between the derivatives at past, present and future instants. The above system (2) can be split into “space-like” and “time-like” parts:
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)
The last equation should be divided by ic.
In [1] is proved that the 4-th equation (3) is a consequence of the first three ones (3.α).
Further on in view of
we obtain
Denoting by
we write the system in the form
(4)
and we have to solve the last system with respect to .
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)
where in view of
we get
(6)

4. An Operator Formulation of the Periodic Problem and Preliminary Assertions

We formulate the main periodic problem: to find a - 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)
Therefore
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.

5. Existence-Uniqueness of the Periodic Problem

Theorem 1 (Main result) Let the following conditions be fulfilled:
1. The initial functions 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.

6. Conclusions

As an immediate consequence we obtain an existence-uniqueness of periodic solution for betatron equation (cf. [14], [27], [38[-[41]). Specific applications we will give in next papers.

References

[1]  Angelov, V. G., 2011, On the original Dirac equations with radiation term., Libertas Mathematica (Texas), 31, 57-86.
[2]  H. A. Lorentz, Die Elektronentheorie. Leipzig, Germany, 1909.
[3]  Dirac, P. A. M., 1938, Classical theory of radiating electrons., Proc. Roy. Soc. (London), A167, 148-169.
[4]  Angelov, V. G., 2015, Two-body problem of classical electrodynamics with radiation terms − derivation of equations (I)., International Journal of Theoretical and Mathematical Physics, 5(5), 119-135.
[5]  Angelov, V. G., 2016, Two-body problem of classical electrodynamics with radiation terms − periodic solutions (II)., International Journal of Theoretical and Mathematical Physics, 6(1), 1-25, 2016.
[6]  Angelov, V. G., 2016, Two-body problem of classical electrodynamics with radiation terms − energy estimation (III)., International Journal of Theoretical and Mathematical Physics, 6(2), 78-85.
[7]  Rohrlich, F., Classical Charged Particles. Foundation of their Theory. Addison-Wesley Publ. Company, Inc. Reading Massachusets, 1965.
[8]  Tetrode, H., 1922, Ueber den wirkungszusammenhang der welt. Eine erweiterung der klassischen dynamic., Zeitschrift fuer Physik, 10, 317-328.
[9]  Fokker, A. D., 1929, Eininvarianter variationssatz fuer die bewegung mehrere elektrischer massenteilchen., Zeitschrift fuer Physik, 58, 386-393.
[10]  Page, L., 1924, Advanced potentials and their applications to atomic models., Phys. Rev., 24, 296-305.
[11]  Wheeler, J. A., and Feynman, R. P., 1945, Interaction with absorber as the mechanism of radiation., Rev. Mod. Physics, 17(2-3), 157-179.
[12]  . Wheeler, J. A., and Feynman, R. P., 1949, Classical Electrodynamics in Terms of direct interparticle Action., Rev. Mod. Physics, 21(3), 425-433.
[13]  D. Ivanenko and A. A. Sokolov, Classical Field Theory. Moscow, 1948 (in Russian).
[14]  L Landau and E. Lifshiz, Field Theory. Moscow, 1948 (in Russian).
[15]  J. D. Jackson, Classical Electrodynamics, New York, London, 1962.
[16]  Schulman, L. S., 1974, Some differential-difference equations containing both advance and retardation., J. Math. Physics, 15(3), 295-298.
[17]  Sorg, M., 1975, Hyperbolic Motion in the finite-size Model of the Radiating Electron., Z. Naturforsch. 30a, 1535-1542.
[18]  Sorg, M., 1978, Retarded Integration in Classical Electrodynamics., Z. Naturforsch. 33 a, 619-620.
[19]  Tabensky, R., 1976, Electrodynamics and the electron equation of motion., Phys. Review D, 13(2), 267-273.
[20]  Moniz, E. J., and Sharp, D. H., 1977, Radiation reaction in non-relativistic quantum electrodynamics., Phys. Rev. D,, 15(10), 2850-2865.
[21]  Deh-phone K. Hsing, and R. D. Driver, “Radiation reaction in Electrodynamics. Dynamical Systems,” in Proc. Univ. Univ. Florida Int. Symposium, Academic Press, 1977, pp. 427-430.
[22]  Maas, W., and Petzold, J., 1978, On the stability of motion of a radiating electron., J. Phys. A: Math. Gen., 11(7), 1211-1219.
[23]  Franca, H. M., Marques, G. C., and da Silva, A. J., 1978, Some aspects of the classical motion of extended charges., Nuovo Cimento, 48 A(1), 65-83.
[24]  Driver, R. D., 1979, Can the future influence the present., Phys. Review D., 19, 1098-1107.
[25]  V. L. Ginsburg, Theoretical Physics and Astrophysics, Moscow, 1981 (in Russian).
[26]  A. A. Sokolov and I. M. Ternov, Relativistic Electron, Nauka, Moscow, 1983 (in Russian).
[27]  I. M. Ternov and V. V. Mikhailin, Synchrotron Radiation. Theory and Experiment, Energoatomizdat, Moscow, 1986 (in Russian).
[28]  A. D. Yaghjian, Relativistic Dynamics of a Charged Shpere, Springer Verlag, 1992.
[29]  W. K. Panofsky and M. Phillips, Classical Electricity and Magnetism, 2nd ed., Addison-Wesley, Reading, Massachusetts, 1969.
[30]  Barut A.O., and Unal, N., “The classical relativistic two-body problem with spin and self-interactions,” in Proc. International Centre for Theoretical Physics, Trieste, 1989.
[31]  D.-A. Deckert and G. Hinrichs, 2015, Electrodynamic two-body problem for prescribing initial date on the straight line, [Online]. Available: .
[32]  G. Bauer, D.-A. Deckert, and D. Durr, 2012, On the existence of dynamics in Wheeler-Feynman electromagnetism, Journal of Applied Mathematics and Physics, 64(4), 1087-1124.
[33]  Angelov V.G., Fixed points in uniform spaces and applications. Cluj University Press, Cluj-Napoca, Romania, 2009.
[34]  Pauli W., Relativitats Theorie, Encyklopedie der Mathematischen Wissenschaften, 19, 1921.
[35]  Synge J. L., 1940, Two-body problem of classical electrodynamics.Proc. Roy. Soc. (London), A177, 118-139.
[36]  V. G. Angelov, A Method for Analysis of Transmission Lines Terminated by Nonlinear Loads, Nova Science, New York, 2014.
[37]  J. J. Livingood, Principles of Cyclic Particle Accelerators, D.Van Nostrand Company, Princeton, New Jersey, 1961.
[38]  M. S. Livingston and J. P. Blewett, Particle Accelerators, Mc-Graw-Hill Book Company, New York, 1962.
[39]  Wille, K., The Physics of Particle Accelerators., Oxford University Press, Inc., US, New York, 2000.