Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions
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arXiv
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| Autori principali: | , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866911087667970048 |
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| author | Bixano, Leonel Matos, Tonatiuh |
| author_facet | Bixano, Leonel Matos, Tonatiuh |
| contents | One of the latest predictions of Einstein's theory is the existence of Wormholes (WH). In this work, we present exact solutions of the Einstein-Maxwell-Dilaton equations representing traversable Wormholes. These solutions satisfy the energy conditions and have a ring singularity satisfying the cosmic censorship of WHs, i.e. we show that, as in previous solutions, geodesics cannot touch the singularity. We find that the most optimal input regions for the first class of solutions traversing these wormholes are near the poles and near the equatorial plane for the second class. We also find that the solution associated with the first class is physically feasible, while for the second class it presents the problem of not being asymptotically flat when considering a dilatonic-type scalar field. Finally, we give examples of realistic astrophysical objects that could fulfill these conditions. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2502_07206 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions Bixano, Leonel Matos, Tonatiuh General Relativity and Quantum Cosmology 83C15, 83E20, 83F05, 53C25, One of the latest predictions of Einstein's theory is the existence of Wormholes (WH). In this work, we present exact solutions of the Einstein-Maxwell-Dilaton equations representing traversable Wormholes. These solutions satisfy the energy conditions and have a ring singularity satisfying the cosmic censorship of WHs, i.e. we show that, as in previous solutions, geodesics cannot touch the singularity. We find that the most optimal input regions for the first class of solutions traversing these wormholes are near the poles and near the equatorial plane for the second class. We also find that the solution associated with the first class is physically feasible, while for the second class it presents the problem of not being asymptotically flat when considering a dilatonic-type scalar field. Finally, we give examples of realistic astrophysical objects that could fulfill these conditions. |
| title | Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions |
| topic | General Relativity and Quantum Cosmology 83C15, 83E20, 83F05, 53C25, |
| url | https://arxiv.org/abs/2502.07206 |