Proca stars in AdS Ellis wormholes
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arXiv
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| Autori principali: | , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866917968024174592 |
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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 |