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This paper classifies BPS and non-BPS orbits for extremal black holes in N = 2 Maxwell–Einstein supergravity theories (MESGT) in five dimensions, demonstrating that attractor equations possess distinct families of solutions with finite Bekenstein–Hawking entropy. The authors analyze the geometry and symmetries of these theories, revealing a correspondence between the theories and Euclidean Jordan algebras of degree three. Additionally, they explore the explicit solutions to the attractor equations and discu

Author

Rafael Frigori

Language

EN