Question 12.71: Use the Larmor formula (Eq. 11.70) and special relativity to...

Use the Larmor formula (Eq. 11.70) and special relativity to derive the Liénard formula (Eq. 11.73).

P=\frac{\mu_{0} q^{2} a^{2}}{6 \pi c}                           (11.70)

P=\frac{\mu_{0} q^{2} \gamma^{6}}{6 \pi c}\left(a^{2}-\left|\frac{ v \times a }{c}\right|^{2}\right)                                (11.73)

The Blue Check Mark means that this solution has been answered and checked by an expert. This guarantees that the final answer is accurate.
Learn more on how we answer questions.

We know that (proper) power transforms as the zeroth component of a 4-vector K^{0}=\frac{1}{c} \frac{d W}{d \tau} . The Larmor formula says that for v=0, \frac{d W}{d \tau}=\frac{1}{4 \pi \epsilon_{0}} \frac{2}{3} \frac{q^{2}}{c^{3}} a^{2} (Eq. 11.70). Can we think of a 4-vector whose zeroth component reduces to this when the velocity is zero?

Well, a^{2} \text { smells like }\left(\alpha^{\nu} \alpha_{\nu}\right), but how do we get a 4-vector in here? How about \eta^{\mu}, whose zeroth component is just c, when v = 0? Try, then:

K^{\mu}=\frac{1}{4 \pi \epsilon_{0}} \frac{2}{3} \frac{q^{2}}{c^{5}}\left(\alpha^{\nu} \alpha_{\nu}\right) \eta_{\mu}

This has the right transformation properties, but we must check that it does reduce to the Larmor formula when v = 0:

\frac{d W}{d t}=\frac{1}{\gamma} \frac{d W}{d \tau}=\frac{1}{\gamma} c K^{0}=\frac{1}{\gamma} c \frac{\mu_{0} q^{2}}{6 \pi c^{3}}\left(\alpha^{\nu} \alpha_{\nu}\right) \eta^{0}, \text { but } \eta^{0}=c \gamma, \text { so } \frac{d W}{d t}=\frac{\mu_{0} q^{2}}{6 \pi c}\left(\alpha^{\nu} \alpha_{\nu}\right) . [Incidentally, this tells us that the power itself (as opposed to proper power) is a scalar. If this had been obvious from the start, we could simply have looked for a Lorentz scalar that generalizes the Larmor formula.]

In Prob. 12.39(b) we calculated \left(\alpha^{\nu} \alpha_{\nu}\right) in terms of ordinary velocity and acceleration:

\begin{aligned}\alpha^{\nu} \alpha_{\nu} &=\gamma^{4}\left[a^{2}+\frac{( v \cdot a )^{2}}{\left(c^{2}-v^{2}\right)}\right]=\gamma^{6}\left[a^{2} \gamma^{-2}+\frac{1}{c^{2}}( v \cdot a )^{2}\right] \\&=\gamma^{6}\left[a^{2}\left(1-\frac{v^{2}}{c^{2}}\right)+\frac{1}{c^{2}}( v \cdot a )^{2}\right]=\gamma^{6}\left\{a^{2}-\frac{1}{c^{2}}\left[v^{2} a^{2}-( v \cdot a )^{2}\right]\right\}\end{aligned}

Now v \cdot a =v a \cos \theta, \text { where } \theta is the angle between v and a, so:

v^{2} a^{2}-( v \cdot a )^{2}=v^{2} a^{2}\left(1-\cos ^{2} \theta\right)=v^{2} a^{2} \sin ^{2} \theta=| v \times a |^{2}.

\alpha^{\nu} \alpha_{\nu}=\gamma^{6}\left(a^{2}-\left|\frac{ v \times a }{c}\right|^{2}\right).

\frac{d W}{d t}=\frac{\mu_{0} q^{2}}{6 \pi c} \gamma^{6}\left(a^{2}-\left|\frac{ v \times a }{c}\right|^{2}\right) , which is Li´enard’s formula (Eq. 11.73).

Related Answered Questions