We proceed to investigate the solutions of generalized supergravity equations (GSE) in three dimensions. Our candidate is the metric of BTZ black hole. It is shown that only the cases with $J=M=0$ and J=0,~ M≠ 0 of the BTZ metric satisfy the GSE. In the former, we find a family of solutions including the field strength H_r φ t=2r/l, the cosmological constant Λ=-1/l², one-form Zμ and a vector field which is obtained to be a linear combination of the directions of the time translation and rotational symmetries. In the latter, the solutions possess the same field strength as before, while the cosmological constant Λ, one-form Zμ and vector field I will be different from the previous case. Finally, we show that the charged black string solution found by Horne and Horowitz, which is Abelian T-dual to the the BTZ black hole solution, can be considered as a solution for the GSE.
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Eghbali et al. (2024) studied this question.
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