arXiv · 2005.14512
No short hair behaviors of ultra-compact stars
Abstract
In the black hole spacetime, a no short hair theorem was proved, which states that the effective radius of black hole hairs must extend beyond the null circular orbit. In the present paper, in the horizonless gravity, we find a similar no short hair behavior that the effective radius of matter fields must also extend beyond the null circular orbit of ultra-compact stars.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Yan Peng. 2020-05-29. No short hair behaviors of ultra-compact stars. https://doi.org/10.1140/epjc%2Fs10052-021-09034-7
Cite the original work for its findings. Save a collection to share your selection of sources.