`BookProof.NavierStokesFlow.nsFlow_energy_conserved` (t : ℝ) (psi : Fin n → ℂ) : star (nsFlowUnitary d t *ᵥ psi) ⬝ᵥ (nsHamiltonian d *ᵥ (nsFlowUnitary d t *ᵥ psi)) = star psi ⬝ᵥ (n

Initializing...

`BookProof.NavierStokesFlow.nsFlow_energy_conserved` (t : ℝ) (psi : Fin n → ℂ) : star (nsFlowUnitary d t *ᵥ psi) ⬝ᵥ (nsHamiltonian d *ᵥ (nsFlowUnitary d t *ᵥ psi)) = star psi ⬝ᵥ (n · Prove2Me