Interaction of cosmological domain walls with large classical objects, like planets and satellites, and the flyby anomaly
De-Chang Dai, Djordje Minic, Dejan Stojkovic

TL;DR
This paper investigates how cosmological domain walls interact with large classical objects like planets and satellites, proposing new methods to detect such walls through observable effects like mass change or energy loss, and explaining the flyby anomaly.
Contribution
It introduces a model for the interaction between domain walls and macroscopic objects, and suggests observational signatures for detecting domain walls via satellite measurements and anomalies.
Findings
Satellites can experience measurable mass changes during wall interactions.
Flyby anomalies can be explained by domain wall interactions.
Matter can induce local vacuum decay near domain walls.
Abstract
Cosmological domain walls can be formed as a result of symmetry breaking at any epoch during the evolution of our universe. We study their interaction with a classical macroscopic object, like Earth or a satellite in Earth's orbit. We set up an action that includes the interaction term between the massive classical object and the scalar field that the domain wall is made of. We use numerical calculations to solve the coupled equations of motion which describe the crossing between the domain wall and the classical object. Depending on the strength of the interaction, relative velocity and size, the object can be either stopped by the wall, or it can pass through it inducing deformations in the wall that cost energy. At the same time, the coupling to the scalar filed might change the object's mass during the crossover. The fact that satellites in Earth's orbit (or planets in Sun's orbit)…
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.
