Lectures on String Theory
Lectures on String Theory
Lectures on String Theory
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– 100 –<br />
Here D α ɛ = ∂ α ɛ − 1 2 ω α ¯ρɛ and ω α is the c<strong>on</strong>necti<strong>on</strong> with torsi<strong>on</strong>:<br />
ω α = ω α (e) + i 4 ¯χ α ¯ρρ β χ β ,<br />
where ω α (e) = − 1 e e αaɛ βγ ∂ β e a γ is the standard composite spin c<strong>on</strong>necti<strong>on</strong> (it has<br />
<strong>on</strong>ly <strong>on</strong>e-n<strong>on</strong>-trivial comp<strong>on</strong>ent in 2dim).<br />
2. Weyl invariance. Let Λ be a bos<strong>on</strong>ic local parameter Λ = Λ(σ, τ). The Weyl<br />
transformati<strong>on</strong>s are<br />
δ Λ X µ = 0 , δ Λ e a α = Λe a α ,<br />
δ Λ ψ µ = − 1 2 Λψµ , δ Λ χ α = 1 2 Λχ α .<br />
3. Super Weyl invariance. Let η be the Majorana spinor. Under the super Weyl<br />
transformati<strong>on</strong>s <strong>on</strong>ly the gravitino transforms as<br />
δ η χ α = ρ α η .<br />
The invarince of the acti<strong>on</strong> easily follows from the identity ρ α ρ β ρ α = 0.<br />
4. Local Lorentz symmetry. Let l be a bos<strong>on</strong>ic local parameter l = l(σ, τ). The<br />
local Lorentz transformati<strong>on</strong>s are<br />
δ l X µ = 0 , δ l e a α = lɛ a be b α ,<br />
δ l ψ µ = 1 2 l¯ρψµ , δ l χ α = 1 2 l¯ρχ α .<br />
5. Reparametrizati<strong>on</strong>s. Let ξ α be a bos<strong>on</strong>ic vector parameter ξ α = ξ α (σ, τ). The<br />
reparametrizati<strong>on</strong>s (diffeomorphisms) are<br />
δ ξ X µ = ξ β ∂ β X µ , δ ξ e a α = ξ β ∂ β e b α + e a β∂ α ξ β ,<br />
δ ξ ψ µ = ξ β ∂ β ψ µ , δ ξ χ α = ξ β ∂ β χ α + χ β ∂ α ξ β .<br />
6.3 Superc<strong>on</strong>formal gauge and supermoduli<br />
The gravitino field is the reducible representati<strong>on</strong> of the Lorentz group. To decompose<br />
it into irreducible representati<strong>on</strong>s <strong>on</strong>e can use the following trick:<br />
χ α = δαχ β β =<br />
(δα β − 1 )<br />
2 ρ αρ β χ β + 1 2 ρ αρ β χ β = 1 2 ρβ ρ α χ β + 1<br />
} {{ } 2 ρ αρ β χ β<br />
˜χ α<br />
Here ˜χ α part is called ρ–traceless because, due to the identity ρ α ρ β ρ α = 0 we get<br />
ρ α ˜χ α = ρ a e α a ˜χ α = ρ a ˜χ a = 0. Indeed the gravitino χ a transforms under local Lorentz