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arxiv gr-qc/9801063 v1 pith:4KB36YUT submitted 1998-01-19 gr-qc

Boson Stars: Early History and Recent Prospects

classification gr-qc
keywords fieldsscalarbosoncasegeneralgravitationalrelativitystars
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Boson stars are descendants of the so-called geons of Wheeler, except that they are built from scalar particles instead of electromagnetic fields. If scalar fields exist in nature, such localized configurations kept together by their self-generated gravitational field can form within Einstein's general relativity. In the case of complex scalar fields, an absolutely stable branch of such non-topological solitons with conserved particle number exists. Our present surge stems from the speculative possibility that these compact objects could provide a considerable fraction of the non-baryonic part of dark matter. In any case, they may serve as a convenient "laboratory" for studying numerically rapidly rotating bodies in general relativity and the generation of gravitational waves.

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Cited by 2 Pith papers

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

  1. A No-Go Theorem for the Mass-Radius Relation of Solitons

    astro-ph.CO 2026-05 unverdicted novelty 7.0

    A no-go theorem excludes Gamma in [0,d] for typical non-topological non-relativistic spherically symmetric solitons, with the same exclusion for barotropic fluid compact objects, ruling out natural soliton explanation...

  2. $\ell$-Boson stars in anti-de Sitter spacetime

    gr-qc 2025-12 unverdicted novelty 5.0

    ℓ-boson stars are constructed and their properties studied in asymptotically anti-de Sitter spacetime.