Reconstructed black hole solutions in the scalar-tensor theory with nonminimal coupling
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| Format: | Preprint |
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2026
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| author | Ernazarov, K. K. |
| author_facet | Ernazarov, K. K. |
| contents | We consider the scalar-tensor theory witn non-minimal coupling in the Jordan frame. The action of the model contains a potential term $U(φ)$, a coupling function $f(φ)$. We explore a reconstruction procedure for a generic static spherically symmetric metric written in the Buchdahl parametrization: $ds^2 = \left(A(u)\right)^{-1}du^2 - A(u)dt^2 + C(u)dΩ^2$, with given $A(u) > 0$ and $C(u) > 0$. The procedure gives the relations for $U(φ(u))$, $f(φ(u))$ and $dφ/du$, which lead to exact solutions to equations of motion with a given metric. A key role in this approach is played by the solutions to a first order linear differential equation for the function $f(φ(u))$. The formalism is illustrated by two examples when: a) the Reissner-Nordström-(Anti-)de Sitter metric and b) the Bocharova-Bronnikov-Melnikov-Bekenstein-(Anti)de-Sitter metric are chosen as a starting point. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2603_22517 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Reconstructed black hole solutions in the scalar-tensor theory with nonminimal coupling Ernazarov, K. K. General Relativity and Quantum Cosmology We consider the scalar-tensor theory witn non-minimal coupling in the Jordan frame. The action of the model contains a potential term $U(φ)$, a coupling function $f(φ)$. We explore a reconstruction procedure for a generic static spherically symmetric metric written in the Buchdahl parametrization: $ds^2 = \left(A(u)\right)^{-1}du^2 - A(u)dt^2 + C(u)dΩ^2$, with given $A(u) > 0$ and $C(u) > 0$. The procedure gives the relations for $U(φ(u))$, $f(φ(u))$ and $dφ/du$, which lead to exact solutions to equations of motion with a given metric. A key role in this approach is played by the solutions to a first order linear differential equation for the function $f(φ(u))$. The formalism is illustrated by two examples when: a) the Reissner-Nordström-(Anti-)de Sitter metric and b) the Bocharova-Bronnikov-Melnikov-Bekenstein-(Anti)de-Sitter metric are chosen as a starting point. |
| title | Reconstructed black hole solutions in the scalar-tensor theory with nonminimal coupling |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2603.22517 |