pith. machine review for the scientific record. sign in

arxiv: 2508.19460 · v2 · submitted 2025-08-26 · 🌀 gr-qc

Recognition: unknown

Search for growing angular modes in ultracompact boson star evolutions

Seppe J. Staelens
Authors on Pith no claims yet
classification 🌀 gr-qc
keywords bosonmodesultracompactadditionallyangularattributedcharacterizationdata
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Boson star-black hole binaries: initial data and head-on collisions

    gr-qc 2026-04 unverdicted novelty 6.0

    A one-body conformal-factor correction stabilizes boson star-black hole initial data, enabling gravitational-wave analysis that shows higher multipoles can discriminate mixed mergers from pure black-hole binaries.