pith. sign in

arxiv: 1712.06231 · v1 · pith:PLM2ZAPEnew · submitted 2017-12-18 · ✦ hep-th · hep-ph

Electromagnetic Radiation in a Semi-Compact Space

classification ✦ hep-th hep-ph
keywords radiationomegainftychargeelectromagneticfourierlimitmode
0
0 comments X
read the original abstract

In this note, we investigate the electromagnetic radiation emitted from a revolving point charge in a compact space. If the point charge is circulating with an angular frequency $\omega_0$ on the $(x,y)$-plane at $z=0$ with boundary conditions, $x \sim x+2 \pi R$ and $y \sim y+2\pi R$, it emits radiation into the $z$-direction of $z$ in $ [-\infty, +\infty]$. We find that the radiation shows discontinuities as a function of $\omega_0 R$ at which a new propagating mode with a different Fourier component appears. For a small radius limit $\omega_0 R \ll 1$, all the Fourier modes except the zero mode on $(x,y)$-plane are killed, but an effect of squeezing the electric field totally enhances the radiation. In the large volume limit $\omega_0 R \rightarrow \infty$, the energy flux of the radiation reduces to the expected Larmor formula.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.