Relativistic Charged Particle

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Total Energy of a Relativistic Charged
Particle moving in and Electromagnetic Field
 

The non-covariant Lagrangian for a charged particle in an electromagnetic field is given by [1]

F is the Coulomb potential and A is the magnetic vector potential. The total time derivative of L is

Using Lagrange’s equations

Eq. (2) can be written as

or

Rearranging terms in Eq. (5) gives

The energy function h is defined as [2]

If h were expressed in terms of canonical momentum then h would be equal to the Hamiltonian H of the system. In terms of h Eq. (6) can be written as

If L, as defined in Eq. (1), is not an explicit function of time then it follows that h = constant, i.e. h is an integral of motion. Evaluating the partial derivative in Eq. (7) yields

The summation in Eq. (7) becomes

Substituting Eq. (10) into the expression for the energy function, i.e. Eq. (7) gives

Thus h = W = the total energy of the particle, hence the name energy function. Further more

E = gm0 is the inertial energy of the particle and V = qF is the potential energy of the particle. E can be written as the sum of the particles kinetic energy, K, and its rest energy, E0.  Then W becomes

If the Lagrangian does not contain the time explicitly then h is conserved i.e. h = constant.


 Derivation of the Lorentz Force
Equation from the Relativistic Lagrangian

Taking the total time derivative of Eq. (9) we get

Taking the partial derivative of Eq. (1) with respect to x gives

Equating Eq. (14) with Eq. (15) gives, according to Lagrange's Equations,

Noting that

Eq. (16) reduces to

Similar results hold for y and z. Thus the final solution is

where

 


The Lorentz Force Equation derived from
 the Covariant Form of the Lorentz Force Equation

The covariant form of the Lorentz Force equation is [3]

where

Consider the time component of Eq. (21), i.e.

Canceling common factor of g from both sides of Eq. (24) reduces that equation to

where E = mc2. Now consider the x component of Eq. (21) by setting a = 1 to get

Eq. (26) simplifies to

Similarly Fy and Fz are obtained from Eq. (20) by setting a = 2 and 3 respectively. The final result is

which is identical the Eq. (19). Thus the following pair of equations is equivalent to the covariant form of Maxwell's equations

If both F and A do not depend on the time explicitly, i.e. F = F (r) and A =A(r), then E = -ÑF and Eq. (25) becomes

It therefore follows that

which is the same result obtained in Section 1 in Eq. (13) if the constant equals the total energy W.


Derivation of the Lorentz
Force Equation from the Covariant Lagrangian

The covariant relativistic Lagrangian L for a charged particle in an electromagnetic field is given by [4]

The covariant Lagrange equations, written in terms of proper time t, is given by [5]

Taking the partial derivative of Eq. (32) with respect to Us we get

The first term can be simplified by noting that

Thus Eq. (34) reduces to

Taking the total derivative of Eq (37) with respect to proper time t gives

To find the second term in the covariant Lagrange equations we take the partial derivative of the covariant Lagrangian, i.e. Eq. (33), with respect to xs to give

Eqs. (38) and (38) are equated to give

Multiply Eq. (40) by gms to give

Eq. (41) is the equation of motion. It can readily be shown by following the same procedure as above that the Lagrangian

will also produce Eq. (41). [6]


References:

[1] Classical Electrodynamics - 3rd Ed., J.D. Jackson, John Wiley & Sons, (1999), page 582 Eq. (12.12).
[2] Classical Mechanics - 3rd Ed., Goldstein, Poole & Safko, Addison Wesley, (2002), page 61 Eq. (2.53).
[3] Ref. 1, page 580 Eq. (12.3).
[4] Ref. 1, page 584 Eq. (12.31).
[5] Ref. 2, page 321 Eq. (7.163).
[6] Ref. 2, page 352 Eq. (7.147).


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