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Chern-Simons vector models and higher spins - Ginzburg ...

Chern-Simons vector models and higher spins - Ginzburg ...

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The Vasiliev’s equationsMaster fields:1. W (x|y, ȳ, z, ¯z) = W µ dx µ 1-form in space-time2. S(x|y, ȳ, z, ¯z) = S α dz α + S ˙α d¯z ˙α 1-form in (z, ¯z)-space3. B(x|y, ȳ, z, ¯z) scalarx µ : spacetime, y α , ȳ ˙α , z α , ¯z ˙α : twistor variables.Collecting W <strong>and</strong> S into the 1-form A = W µ dx µ + S α dz α + S ˙α d¯z ˙α ,Vasiliev’s equation can be written asdA + A ∗ A = V(B ∗ κ)dz 2 + ¯V(B ∗ ¯κ)d¯z 2dB + A ∗ B − B ∗ π(A) = 0Simone Giombi (PI) <strong>Chern</strong>-<strong>Simons</strong> <strong>and</strong> <strong>higher</strong> <strong>spins</strong> Lebedev Inst., Jun 1 2012 6 / 24

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