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Class of Eistein-Maxwell Dilatons
General Relativity and Quantum Cosmology · Submitted 28 Aug 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Most of the known solutions of charged and dilatonic black holes are contained as special cases and can be non-trivially generalized in different ways.
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The abstract, sentence by sentence
The functional potential formalism is used to analyze stationary axisymmetric spaces in the Einstein-Maxwell-Dilaton theory. Performing a Legendre transformation, a ``Hamiltonian''is obtained, which allows to rewrite the dynamical equations in terms of three complex functions only. Using an ansatz resembling the one used by the harmonic maps ansatz, we express these three functions in terms of the harmonic parameters, studying the cases where these parameters are real, and when they are complex. For each case, the set of equations in terms of these harmonic parameters is derived, and several classes of solutions to the Einstein-Maxwell with arbitrary coupling constant to a dilaton field are presented. Most of the known solutions of charged and dilatonic black holes are contained as special cases and can be non-trivially generalized in different ways.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The functional potential formalism is used to analyze stationary axisymmetric spaces in the Einstein-Maxwell-Dilaton theory. | method 0.79 | 0.75 | 0.05 | asserted 1.00 |
| s1 | Performing a Legendre transformation, a ``Hamiltonian''is obtained, which allows to rewrite the dynamical equations in terms of three complex functions only. | method 0.98 | 0.91 | 0.06 | asserted 1.00 |
| s2 | Using an ansatz resembling the one used by the harmonic maps ansatz, we express these three functions in terms of the harmonic parameters, studying the cases where these parameters are real, and when they are complex. | method 0.95 | 0.92 | 0.06 | asserted 1.00 |
| s3 | For each case, the set of equations in terms of these harmonic parameters is derived, and several classes of solutions to the Einstein-Maxwell with arbitrary coupling constant to a dilaton field are presented. | result 0.65 | 0.93 | 0.38 | asserted 1.00 |
| s4 | Most of the known solutions of charged and dilatonic black holes are contained as special cases and can be non-trivially generalized in different ways. | interpretation 0.50 | 0.71 | 0.52 | asserted 0.94 |
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Original abstract
The functional potential formalism is used to analyze stationary axisymmetric spaces in the Einstein-Maxwell-Dilaton theory. Performing a Legendre transformation, a ``Hamiltonian''is obtained, which allows to rewrite the dynamical equations in terms of three complex functions only. Using an ansatz resembling the one used by the harmonic maps ansatz, we express these three functions in terms of the harmonic parameters, studying the cases where these parameters are real, and when they are complex. For each case, the set of equations in terms of these harmonic parameters is derived, and several classes of solutions to the Einstein-Maxwell with arbitrary coupling constant to a dilaton field are presented. Most of the known solutions of charged and dilatonic black holes are contained as special cases and can be non-trivially generalized in different ways.
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References
How the literature uses it
3 arXiv papers cite this in 5 sentences
Papers citing it · 3 sentences without a confident label
Uses its method or tool 1 paper
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In this work, we adopt the potential-space metric that has been used in the analyses of Refs. [ref] .
Potential Space Symmetries in Ernst-like Formulations of Einstein-Maxwell/ModMax-Scalar field Theories · Metric on the space of potentials and manifest symmetries · 0.93
Cites it as background 1 paper
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This stringy extension of the Reissner-Nordström (RN) BH has attracted an enormous attention, finding a variety of interesting applications, $e.g.$ [ref] .
De-singularizing the extremal GMGHS black hole via higher derivatives corrections · Introduction · 0.97
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