Index saddle for supersymmetric F1-P black ring
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arXiv
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| Format: | Preprint |
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2026
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| _version_ | 1866914610741772288 |
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| author | Dharanipragada, Pavan Punia, Gurmeet Singh Virmani, Amitabh |
| author_facet | Dharanipragada, Pavan Punia, Gurmeet Singh Virmani, Amitabh |
| contents | We construct the index saddle for the supersymmetric F1--P black ring. Our construction proceeds by taking a supersymmetric limit of a non-supersymmetric doubly spinning F1--P black ring. We express the resulting saddle as a three-center Bena--Warner solution. The black ring saddle possesses a finite-area event horizon, yet the two-derivative index vanishes. The solution is singular on certain subspaces of the horizon, where higher-derivative corrections are expected to become important. We argue that, once such corrections are taken into account, the solution can yield a finite result. In particular, we present a scaling analysis showing that the index agrees with the microscopic result, up to an overall numerical constant that cannot be fixed by the scaling argument alone. This analysis applies only within a restricted region of parameter space, whose full significance is not yet fully understood. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2601_04624 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Index saddle for supersymmetric F1-P black ring Dharanipragada, Pavan Punia, Gurmeet Singh Virmani, Amitabh High Energy Physics - Theory General Relativity and Quantum Cosmology We construct the index saddle for the supersymmetric F1--P black ring. Our construction proceeds by taking a supersymmetric limit of a non-supersymmetric doubly spinning F1--P black ring. We express the resulting saddle as a three-center Bena--Warner solution. The black ring saddle possesses a finite-area event horizon, yet the two-derivative index vanishes. The solution is singular on certain subspaces of the horizon, where higher-derivative corrections are expected to become important. We argue that, once such corrections are taken into account, the solution can yield a finite result. In particular, we present a scaling analysis showing that the index agrees with the microscopic result, up to an overall numerical constant that cannot be fixed by the scaling argument alone. This analysis applies only within a restricted region of parameter space, whose full significance is not yet fully understood. |
| title | Index saddle for supersymmetric F1-P black ring |
| topic | High Energy Physics - Theory General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2601.04624 |