Axially symmetric ghost stars
arXiv:2506.05114 · doi:10.1140/epjc/s10052-025-14351-2
Abstract
We present static axially symmetric fluid distributions not producing gravitational field outside their boundaries (i.e. fluid sources which match smoothly on the boundary surface to Minkowski space-time). These solutions provide further examples of ghost stars. A specific model is fully described, and its physical and geometrical properties are analyzed in detail. This includes the multipole moment structure of the source and its complexity factors, both of which vanish for our solution.
9 pages, 7 figures. arXiv admin note: text overlap with arXiv:2304.12640
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