Search for growing angular modes in ultracompact boson star evolutions
Abstract
Abstract Recent fully non-linear simulations of ultracompact spherically symmetric boson stars have presented evidence for their long-term stability. All observed dynamics could be mainly attributed to the fundamental radial mode. In this work, we additionally decompose some of the data in spherical harmonics, providing a first step towards the characterization of non-spherical modes present.
Fields of Study & Subjects
Pulsars and Gravitational Waves Research
Astronomy and Astrophysical Research
Cosmology and Gravitation Theories
Publication details
- Journal / source
- Journal of Physics Conference Series
- Publisher
- IOP Publishing
- Volume
- 3177
- Issue
- 1
- Pages
- 012046–012046
- Publication date
- 1 February 2026