Some Studies on the Lorentz Theory of Radiation Reaction in Relation to a Charged Particle Acted on by a Constant Force in a Finite Time Interval

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**Subject Areas:** **Theoretical Physics**

1. Introduction

It is well known fact that the theory of radiation reaction in electrodynamics as worked out by Lorentz [1] (actually by Lorentz, Abraham and Dirac) has solutions, which exhibits a runaway nature and/or non-causal pre- acceleration. In fact the non-causal pre-acceleration without runaway makes more sense and in this paper we will only be concerned with this solution of the equation of motion. It is generally believed that the non-causal pre-acceleration exists for a short duration (typically seconds for the electron) when it becomes comparable in magnitude to that of the actual acceleration and hence can never be detected in an experiment. Below we study the case of a charged particle when it is moving under the influence of a constant force preferably of a non-electromagnetic origin for a finite time duration and compare it with the dynamics of an uncharged particle of equal mass under the action of the same force. The second particle of course does not experience radiation reaction. Also we put a different initial condition and try to find out if there is some measurable parameter which detects pre-acceleration in an experiment. In the last section we discuss some difficulties with the attempts to eliminate pre-acceleration theoretically as they exist in literature [2] . Only non-relativistic dynamical equations have been used for the present and that too for one dimensional motion.

2. The Dynamical Equation of the Charged Particle with Some Initial Condition and Acted on by a Constant Force f_{ext} from 0 to t Seconds

From Equation (1.1) of ref. [1] we can write the equation of motion in one dimension as

, (1)

where is about sec. for the electron and m is its mass. From Equations (1.2) and (1.3) of the same reference we can write the pre accelerated solution without runaway as

. (2)

For the special case of to be a constant between and we can represent it mathematically in terms of the unit step function as

, (3)

where for and for. We also prefer to be of non electromagnetic origin so that it can act equally well on charged and uncharged particles alike. This restriction can be relaxed when uncharged particles are not under consideration as we see in Section 3. Thus for of the type described by Equation (3) the acceleration from Equation (2) becomes

(4)

The time derivative of acceleration and the velocity respectively are

(5)

and

(6)

The constant K will be zero if. For the case of the uncharged particle of the same mass which we have already assumed to be accelerated by the same force in accordance with Newton’s laws the velocity is

(constant), (7)

where the subscript un of v denotes that it is the velocity of the uncharged particle. For we again get the constant. With this set of initial conditions it is easy to show that the final velocity attained at is given identically for the two particles to be

. (8)

Thus in the Lorentz theory of radiation reaction the change in kinetic energy of a radiating charged particle is equal to that of a non radiating uncharged particle when acted on by equal external forces in equal intervals of time. This fact can be determined in an experiment. The energy radiated out by the charged particle is given by the Larmor’s formula

. (9)

One can easily show that this comes from the extra work done by when it is applied on the charged particle as compared to when it is applied on the uncharged one in the time interval 0 to t.

3. Possible Means to Experimentally Detect Pre-Acceleration

In this section we study only the dynamics of charged particles so the restriction on to be of non electromagnetic origin may be relaxed. The initial condition is changed from to some finite velocity. Let us for example take the initial velocity to be the same as that of the final velocity attained by the particle in the last section that is. This becomes the new value of the constant K in Equation (6). Now we use the energy conservation equation given by Gron (see Equation (2.1) of ref. [1] ) in the non relativistic limit

(10)

In the non relativistic limit is the Schott force and for the one dimensional problem of Section 2 and the initial condition for the time we have

. (11)

From these and using the values of and v from Equations (5) and (6) we get the value of the change in

kinetic energy from to zero to be

. (12)

Since this change in kinetic energy of the particle beam before is almost equal to the magnitude of the radiated energy in the interval that is during the interval when a constant force is applied (compare Equations (9) and (12)), it must be experimentally detectable. This can be done by spectral methods to detect the shift in kinetic energy of the electrons (particles) in the beam when measured at as compared to the value much before this time. In fact it will confirm or disprove the Lorentz, Abraham and Dirac theory of radiation reaction and the pre acceleration associated with it.

4. Theoretical Attempts to Cancel Pre-Acceleration in the Lorentz Theory of Radiation Reaction

Yaghjian [2] had tried to modify the existing equation of motion of the Lorentz theory of radiation reaction in a way such that pre-acceleration is excluded. He writes (see Equation (8.34) of Ref. [2] ) in place of Equation (1) of the present paper the following equation of motion expressed as per the notations used in this paper

(13)

This will first of all violate energy conservation as expressed by Equation (10) and there is no simple way to get around this difficulty if other aspects of Lorentz theory are to be kept intact after. Also the solution given for this equation of motion which is stated as

for

for

has some features which makes it behave differently from the expression for acceleration as given by Equation (2) near. This is because the function in the expression above rapidly falls towards zero as causing some sort of “overshoot” if the force is of the form given by Equation (3) and may have some experimentally observed consequences especially when t (please refer to the previous sections) is small.

References

[1] Gron, O. (2012) Electrodynamics of Radiating Charges. Advances in Mathematical Physics, 2012, Article ID: 528631.

http://dx.doi.org/10.1155/2012/528631

[2] Yaghjian, A.D. (1992) Relativistic Dynamics of a Charged Sphere. Springer-Verlag, New York.