New method to generate exact scalar-tensor solutions - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue Physical Review D Année : 2019

New method to generate exact scalar-tensor solutions

Résumé

A new method is proposed, that establishes a one to one correspondance between the whole set of static axially symmetric vacuum general relativity solutions and a specific class of stationary axially symmetric scalar-Einstein (Rab=∂aφ∂bφ) solutions for any mass and angular momentum. The method explicitly takes advantage of the Kerr metric Ricci flatness. This also results in a class of stationary axially symmetric vacuum, ie Kerrlike, Brans-Dicke solutions. A particular solution, that is asymptotically flat, is more closely considered. It converges to Kerr for a vanishing scalar charge, but fails to converge to the Fisher-Janis-Newman-Winicour solution for a vanishing “rotation parameter.” This solution exhibits a set of singular points, with a naked subset having a ringlike structure.
Fichier principal
Vignette du fichier
10.1103PhysRevD.100.024051.pdf (256.78 Ko) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte

Dates et versions

hal-01974756 , version 1 (16-06-2023)

Identifiants

Citer

Bertrand Chauvineau. New method to generate exact scalar-tensor solutions. Physical Review D, 2019, 100 (2), pp.024051. ⟨10.1103/PhysRevD.100.024051⟩. ⟨hal-01974756⟩
58 Consultations
10 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More