Semiclassical approach to the decay of protons in circular motion under the influence of gravitational fields
Douglas Fregolente, George E. A. Matsas (Sao Paulo, IFT), Daniel A. T., Vanzella (Sao Paulo U., Sao Carlos)

TL;DR
This paper explores the decay of protons in circular geodesic motion near neutral compact objects using a semiclassical method, comparing results with electromagnetic decay scenarios and providing consistency analyses.
Contribution
It introduces a semiclassical framework to analyze proton decay in gravitational fields, extending previous electromagnetic-focused studies.
Findings
Decay rates depend on gravitational field strength
Emitted power varies with orbital parameters
Results align with theoretical expectations for gravitational decay
Abstract
We investigate the possible decay of protons in geodesic circular motion around neutral compact objects. Weak and strong decay rates and the associated emitted powers are calculated using a semi-classical approach. Our results are discussed with respect to distinct ones in the literature, which consider the decay of accelerated protons in electromagnetic fields. A number of consistency checks are presented along the paper.
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.
