Proca stars in AdS Ellis wormholes

Fuente: arXiv
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Autori principali: Li, Gen, Hao, Chen-Hao, Su, Xin, Wang, Yong-Qiang
Natura: Preprint
Pubblicazione: 2025
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author Li, Gen
Hao, Chen-Hao
Su, Xin
Wang, Yong-Qiang
author_facet Li, Gen
Hao, Chen-Hao
Su, Xin
Wang, Yong-Qiang
contents In this paper, we study Proca stars in asymptotically anti-de Sitter (AdS) Ellis wormholes. This study distinguishes itself from the analysis of the Proca stars in asymptotically flat spacetimes. In the AdS Ellis wormhole background, the mass of the wormhole solutions vanishes. Consequently, we employ numerical techniques to investigate in detail the impact of the cosmological constant on both the matter field and the wormhole geometry, while categorizing the solutions in accordance with the symmetries of the Proca field. The results show that when the cosmological constant decreases, not only does the characteristic spiral behavior of the Proca star solutions, namely the charge-frequency relation $Q$-$ω$, gradually disappear, but the throat or both sides of the wormhole may also develop a ``horizon", presenting a ``black bounce" characteristic.
format Preprint
id arxiv_https___arxiv_org_abs_2503_19810
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Proca stars in AdS Ellis wormholes
Li, Gen
Hao, Chen-Hao
Su, Xin
Wang, Yong-Qiang
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this paper, we study Proca stars in asymptotically anti-de Sitter (AdS) Ellis wormholes. This study distinguishes itself from the analysis of the Proca stars in asymptotically flat spacetimes. In the AdS Ellis wormhole background, the mass of the wormhole solutions vanishes. Consequently, we employ numerical techniques to investigate in detail the impact of the cosmological constant on both the matter field and the wormhole geometry, while categorizing the solutions in accordance with the symmetries of the Proca field. The results show that when the cosmological constant decreases, not only does the characteristic spiral behavior of the Proca star solutions, namely the charge-frequency relation $Q$-$ω$, gradually disappear, but the throat or both sides of the wormhole may also develop a ``horizon", presenting a ``black bounce" characteristic.
title Proca stars in AdS Ellis wormholes
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2503.19810