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Statut |
Confirmé |
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Série |
SEM-GRECO |
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Domaines |
gr-qc |
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Date |
Lundi 2 Novembre 2020 |
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Heure |
11:00 |
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Institut |
IAP |
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Salle |
zoom details: contact pitrou@iap.fr |
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Nom de l'orateur |
Anson |
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Prenom de l'orateur |
Timothy |
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Addresse email de l'orateur |
timothy [dot] anson [at] th [dot] u-psud [dot] fr |
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Institution de l'orateur |
LPT Orsay |
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Titre |
Disforming the Kerr metric |
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Résumé |
Starting from a recently constructed stealth Kerr solution of higher order scalar tensor theory involving scalar hair, we analytically construct disformal versions of the Kerr spacetime with a constant degree of disformality and a regular scalar field. While the disformed metric has only a ring singularity and asymptotically is quite similar to Kerr, it is found to be neither Ricci flat nor circular. Non-circularity has far reaching consequences on the structure of the solution. As we approach the rotating compact object from asymptotic infinity we find a static limit ergosurface similar to the Kerr spacetime with an enclosed ergoregion. However, the stationary limit of infalling observers is found to be a timelike hypersurface. A candidate event horizon is found in the interior of this stationary limit surface. It is a null hypersurface generated by a null congruence of light rays which are no longer Killing vectors. Under a mild regularity assumption, we find that the candidate surface is indeed an event horizon and the disformed Kerr metric is therefore a black hole quite distinct from the Kerr solution. |
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Numéro de preprint arXiv |
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Commentaires |
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