Electromagnetic back-reaction from currents on a straight string
Jeremy M. Wachter, Ken D. Olum

TL;DR
This paper analyzes how electromagnetic back-reaction prevents infinite current growth on a straight superconducting cosmic string, showing that fields and currents decay to avoid divergence, with implications for gravitational effects.
Contribution
It provides a detailed calculation of electromagnetic back-reaction on a cosmic string, demonstrating the natural damping mechanism preventing divergence of currents.
Findings
Electromagnetic fields and currents decay rapidly enough to prevent divergence.
Back-reaction effectively dampens the current asymptotically to zero.
Implications discussed for gravitational analogs.
Abstract
Charge carriers moving at the speed of light along a straight, superconducting cosmic string carry with them a logarithmically divergent slab of electromagnetic field energy. Thus no finite local input can induce a current that travels unimpeded to infinity. Rather, electromagnetic back-reaction must damp this current asymptotically to nothing. We compute this back-reaction and find that the electromagnetic fields and currents decline exactly as rapidly as necessary to prevent a divergence. We briefly discuss the corresponding gravitational situation.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
