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We detail the construction of the most general asymptotically flat, stationary, rotating, non-extremal, dyonic black hole of the four-dimensional N=2 supergravity coupled to 3 vector multiplets that describes the STU model.
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1998
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2009
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P. Lévay, “ S T U STU black holes as four-qubit systems,” Phys. Rev. D 82
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2011
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2011
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2012
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2012
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