Acausal exact vacuum solutions in nonlocal gravity
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arXiv
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| Hauptverfasser: | , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866917454403338240 |
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| author | Zhao, Zhe Modesto, Leonardo Bambi, Cosimo |
| author_facet | Zhao, Zhe Modesto, Leonardo Bambi, Cosimo |
| contents | Nonlocal gravity is a promising super-renormalizable or finite quantum gravity theory consistent with unitarity. In this paper, we focus on the classical equations of motion and explicitly show that a particular subclass of Gödel-type Universes, where closed time-like curves are allowed, is an exact solution of nonlocal gravity in vacuum. The result is consistent with a well defined theory at quantum level, but it is realized only with a special, although large, class of nonlocal form factors. Therefore, by itself the renormalizability requirement is not a sufficient guiding principle in vacuum whether we want to avoid the causality violation. From the physical point of view, the causality violation takes place from the non locality fundamental scale to macroscopic scales. Therefore, it is the presence of matter to break the classical degeneracy between the Minkowski and the Gödel Universe. Finally, we have shown that at the non-perturbative quantum level the transition from a flat to a Gödel Universe is ridiculously small. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_01413 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Acausal exact vacuum solutions in nonlocal gravity Zhao, Zhe Modesto, Leonardo Bambi, Cosimo General Relativity and Quantum Cosmology Nonlocal gravity is a promising super-renormalizable or finite quantum gravity theory consistent with unitarity. In this paper, we focus on the classical equations of motion and explicitly show that a particular subclass of Gödel-type Universes, where closed time-like curves are allowed, is an exact solution of nonlocal gravity in vacuum. The result is consistent with a well defined theory at quantum level, but it is realized only with a special, although large, class of nonlocal form factors. Therefore, by itself the renormalizability requirement is not a sufficient guiding principle in vacuum whether we want to avoid the causality violation. From the physical point of view, the causality violation takes place from the non locality fundamental scale to macroscopic scales. Therefore, it is the presence of matter to break the classical degeneracy between the Minkowski and the Gödel Universe. Finally, we have shown that at the non-perturbative quantum level the transition from a flat to a Gödel Universe is ridiculously small. |
| title | Acausal exact vacuum solutions in nonlocal gravity |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2605.01413 |