Geometry and Thermodynamics of Black Holes in Magnetic Fields ...
Geometry and Thermodynamics of Black Holes in Magnetic Fields ...
Geometry and Thermodynamics of Black Holes in Magnetic Fields ...
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SU(2, 1) Transformations, <strong>and</strong> Magnetisation• The scalar sigma model metricdΣ 2 = dϕ 2 + e 2ϕ [dχ 2 + dψ 2 ] + e 4ϕ (dσ − 2χdψ) 2˜is CP 2 = SU(2, 1)/U(2), the non-compact (negative curvature)version <strong>of</strong> CP 2 . Def<strong>in</strong><strong>in</strong>g matrices E b a with just a 1 atrow a, column b, <strong>and</strong> H = E 0 0 − E 2 2 , we can parameterise acoset representative, <strong>and</strong> SU(2, 1) element, asV = e ϕH e −2i σE 0 2 e√2χ(E0 1 +E 2) 1 e −i √ 2ψ(E 1 0 −E 2) 1 .We haveV † ηV = η , η =⎛⎜⎝0 0 −10 1 0−1 0 0⎞⎟⎠ ,with η be<strong>in</strong>g the <strong>in</strong>variant metric <strong>of</strong> SU(2, 1). The Lagrangiancan be written as L 3 = R − tr(M −1 ∂M) 2 where M = V † V.L 3 is manifestly <strong>in</strong>variant under M −→ M ′ = U † MU where Uis any constant SU(2, 1) matrix, obey<strong>in</strong>g U † ηU = η.