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Boson stars with negative cosmological constant

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arxiv gr-qc/0309131 v1 pith:APXNQUDZ submitted 2003-09-29 gr-qc hep-th

Dumitru Astefanesei , Eugen Radu This is my paper · ORCID
classification gr-qchep-th
keywords bosoncosmologicalconstantdimensionalpropertiessolutionsstaranti-de
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abstract

We consider boson star solutions in a $D$-dimensional, asymptotically anti-de Sitter spacetime and investigate the influence of the cosmological term on their properties. We find that for $D>4$ the boson star properties are close to those in four dimensions with a vanishing cosmological constant. A different behavior is noticed for the solutions in the three dimensional case. We establish also the non-existence of static, spherically symmetric black holes with a harmonically time-dependent complex scalar field in any dimension greater than two.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 99 citations worldwide. Full citation record

  1. Light Rings, Accretion Disks and Shadows of Hayward Boson Stars

    gr-qc 2025-07 unverdicted novelty 5.0 of 10

    Numerical construction of Hayward boson stars shows that frozen states produce Schwarzschild-like shadows with no extra photon rings while non-frozen states show multiple photon rings inside the shadow.

  2. Dynamical Boson Stars

    gr-qc 2012-02 unverdicted novelty 2.0 of 10

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

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