Tutorial 1: The GCT Chasm I
summary
Claims that a strengthened permanent-versus-determinant conjecture forces derandomization of Noether’s Normalization for the orbit closure of the determinant, moving the problem from current XSPACE/EXPSPACE down to quasi-determinant (quasi-P) under that conjecture and standard tools (GRH, hardness-to-randomness, Kaltofen factorization). Evidence: the orbit boundary contains “bad exterior points” produced by Newton degeneration that cause exponential circuit-size blowup (beyond the known N^2 lower bound), tied to representation-theoretic tame/wild behavior and Milnor–Thom style geometry. Consequences include potential PH collapse if the chasm cannot be crossed.
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chapters (10)
- 0:00Start
- 1:16The main reference
- 1:46The beginning of GCT
- 9:44The permanent vs. determinant problem
- 16:54What if the GCT chasm cannot be crossed?
- 19:48Outline of the talk
- 23:17The orbit closures
- 24:32The reformulation in terms of orbit closures
- 26:24What lies on the border of G det(Y)?
- 52:49Noether's Normalization Lemma [Hilbert]
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