A class of space-times of non-rigidly rotating dust
Lukasz Bratek, Joanna Jalocha, Marek Kutschera

TL;DR
This paper presents a new class of exact solutions in General Relativity describing differentially rotating dust space-times with asymptotic flatness, positive mass, and potential angular momentum, distinct from previous models.
Contribution
It introduces a novel class of solutions for rotating dust in General Relativity, expanding understanding of such space-times with unique properties.
Findings
Existence of asymptotically flat space-times with positive mass
Some solutions possess non-zero total angular momentum
Flow differs from previously known solutions like van Stockum's
Abstract
We find a class of exact solutions of differentially rotating dust in the framework of General Relativity. There exist asymptotically flat space-times of the flow with positive mass function that for radii sufficiently large is monotonic and tends to zero at infinity. Some of the space-times may have non-vanishing total angular momentum. The flow is essentially different from another exactly solvable flow described by van Stockum line element.
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.
Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Solar and Space Plasma Dynamics
