Axially symmetric ghost stars

Fuente: arXiv
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Auteurs principaux: Herrera, L., Hernandez-Pastora, J. L., Ospino, J., Di Prisco, A.
Format: Preprint
Publié: 2025
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author Herrera, L.
Hernandez-Pastora, J. L.
Ospino, J.
Di Prisco, A.
author_facet Herrera, L.
Hernandez-Pastora, J. L.
Ospino, J.
Di Prisco, A.
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2506_05114
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Axially symmetric ghost stars
Herrera, L.
Hernandez-Pastora, J. L.
Ospino, J.
Di Prisco, A.
General Relativity and Quantum Cosmology
Solar and Stellar Astrophysics
Mathematical Physics
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.
title Axially symmetric ghost stars
topic General Relativity and Quantum Cosmology
Solar and Stellar Astrophysics
Mathematical Physics
url https://arxiv.org/abs/2506.05114