The Approach of

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Collaborators and some publications Introduction Action of the Approach Yukawa couplings and scalar fields The spinor represent The Einstein action for a free gravitational field is assumed to be linear in the curvature L g = E (α ω R + ˜α˜R), R = f α[a f βb] (ω abα,β − ω caα ω c bβ), ˜R = f α[a f βb] (˜ω abα,β − ˜ω caα ˜ω c bβ), with E = det(e a α) and f α[a f βb] = f αa f βb − f αb f βa . N.S. Mankoč Borštnik, Cape Town 2010, 01-06 February University of Ljubljana The Approach Unifying spins and charges
Collaborators and some publications Introduction Action of the Approach Yukawa couplings and scalar fields The spinor represent Variation of the action brings for ω abα ω abα = − 1 2E − − e { eα ¯Ψ 4 1 d − 2 { e eα e bγ ∂ β (Ef γ[e f β a]) + e eα e aγ ∂ β (Ef γ [bf βe] ) − e eα e e ( γ ∂ β Ef γ [a f β ) } b] ( γ e S ab + 3i ) 2 (δe b γ a − δaγ e b ) [ 1 ( ) {e aα E ed γ∂ β Ef γ [df β b] } Ψ + 1 ] 2 ¯Ψγ d S db Ψ [ 1 ) − e bα E ed γ∂ β (Ef γ [df β a] + 1 }] 2 ¯Ψγ d S da Ψ N.S. Mankoč Borštnik, Cape Town 2010, 01-06 February University of Ljubljana The Approach Unifying spins and charges
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