Introduction to Electrodynamics · Problem 12.37

Electrodynamics and Relativity — David J. Griffiths

Physics · relativistic-dynamics

Problem

In classical mechanics, Newton's law can be written in the more familiar form F=ma\mathbf{F} = m\mathbf{a}. The relativistic equation, F=dp/dt\mathbf{F} = d\mathbf{p}/dt, cannot be so simply expressed. Show, rather, that F=m1−u2/c2[a+u(u⋅a)c2−u2],(12.74)\mathbf{F} = \frac{m}{\sqrt{1-u^2/c^2}}\left[\mathbf{a} + \frac{\mathbf{u}(\mathbf{u}\cdot\mathbf{a})}{c^2 - u^2}\right], \tag{12.74} where a≡du/dt\mathbf{a} \equiv d\mathbf{u}/dt is the ordinary acceleration.

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