Ultrarelativistic circular orbits of spinning particles in a Schwarzschild field
Roman Plyatsko
TL;DR
This paper investigates the behavior of ultrarelativistic spinning particles in a Schwarzschild gravitational field, focusing on their circular orbits and potential electromagnetic radiation emitted by such particles near black holes.
Contribution
It provides a detailed analysis of ultrarelativistic circular orbits of spinning particles using Mathisson-Papapetrou equations and estimates their synchrotron radiation in black hole environments.
Findings
Ultrarelativistic spinning particles can maintain circular orbits in Schwarzschild fields.
Estimated synchrotron radiation from these particles could be detectable near black holes.
The study offers insights into particle dynamics and radiation in strong gravitational fields.
Abstract
Ultrarelativistic circular orbits of spinning particles in a Schwarzschild field described by the Mathisson-Papapetrou equations are considered. The preliminary estimates of the possible synchrotron electromagnetic radiation of highly relativistic protons and electrons on these orbits in the gravitational field of a black hole are presented
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.