Levitating atmospheres around naked singularities
Ronaldo S. S. Vieira, W{\l}odek Klu\'zniak

TL;DR
This paper explores the existence of levitating atmospheres around naked singularities, where gravity becomes repulsive, preventing matter from reaching the singularity and forming stable, radiation-free suspended atmospheres.
Contribution
It introduces the concept of levitating atmospheres around naked singularities, highlighting their properties and differences from radiation-supported atmospheres.
Findings
Gravity becomes effectively repulsive near naked singularities
Levitating atmospheres form due to repulsive gravity effects
Maximum density occurs at a specific radius within the atmosphere
Abstract
For a wide class of spherically symmetric naked singularities there is a sphere within which gravity is effectively repulsive. In such spacetimes accreting matter cannot reach the singularity and will instead form a levitating atmosphere, which is kept suspended by gravity alone. The density of the atmosphere has a maximum at a definite radius. In its qualitative properties the atmosphere is analogous to the recently discussed atmospheres that are supported by radiation pressure above luminous neutron stars, however for the levitating atmospheres around a naked singularity no radiation need be present.
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 · Astrophysical Phenomena and Observations · Black Holes and Theoretical Physics
