English

Electromagnetic Radiation in a Semi-Compact Space

High Energy Physics - Theory 2018-02-14 v1 High Energy Physics - Phenomenology

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 ω0\omega_0 on the (x,y)(x,y)-plane at z=0z=0 with boundary conditions, xx+2πRx \sim x+2 \pi R and yy+2πRy \sim y+2\pi R, it emits radiation into the zz-direction of zz in [,+] [-\infty, +\infty]. We find that the radiation shows discontinuities as a function of ω0R\omega_0 R at which a new propagating mode with a different Fourier component appears. For a small radius limit ω0R1\omega_0 R \ll 1, all the Fourier modes except the zero mode on (x,y)(x,y)-plane are killed, but an effect of squeezing the electric field totally enhances the radiation. In the large volume limit ω0R\omega_0 R \rightarrow \infty, the energy flux of the radiation reduces to the expected Larmor formula.

Keywords

Cite

@article{arxiv.1712.06231,
  title  = {Electromagnetic Radiation in a Semi-Compact Space},
  author = {Satoshi Iso and Noriaki Kitazawa and Sumito Yokoo},
  journal= {arXiv preprint arXiv:1712.06231},
  year   = {2018}
}

Comments

to be published in PLA

R2 v1 2026-06-22T23:21:00.674Z