Spherically symmetric space-times in generalized hybrid metric-Palatini gravity
arXiv:2109.01794 · doi:10.1134/S0202289321040046
Abstract
We discuss vacuum static, spherically symmetric asymptotically flat solutions of the generalized hybrid metric-Palatini theory of gravity (generalized HMPG) suggested by Böhmer and Tamanini, involving both a metric and an independent connection ; the gravitational field Lagrangian is an arbitrary function of two Ricci scalars, obtained from and obtained from . The theory admits a scalar-tensor representation with two scalars and and a potential whose form depends on . Solutions are obtained in the Einstein frame and transferred back to the original Jordan frame for a proper interpretation. In the completely studied case , generic solutions contain naked singularities or describe traversable wormholes, and only some special cases represent black holes with extremal horizons. For , some examples of analytical solutions are obtained and shown to possess naked singularities. Even in the cases where the Einstein-frame metric is found analytically, the scalar field equations need a numerical study, and if contains a horizon, in the Jordan frame it turns to a singularity due to the corresponding conformal factor.
arXiv comment18 pages, 7 figures
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