Natural-gradient methods markedly accelerate the training of Physics-Informed Neural Networks (PINNs), yet their Gauss–Newton update must be solved in the parameter space, incurring a prohibitive time complexity, where is the number of network trainable weights. We show that exactly the same step can instead be formulated in a generally smaller residual space of size , where each residual class (e.g. PDE interior, boundary, initial data) contributes collocation points of output dimension . Building on this insight, we introduce (D-NGD). D-NGD computes the Gauss–Newton step in residual space, augments it with a geodesic-acceleration correction at negligible extra cost, and provides both a dense direct solver for modest and a Nystrom-preconditioned conjugate-gradient solver for larger . Experimentally, D-NGD scales second-order PINN optimization to networks with up to 12.8 million parameters, delivers one- to three-order-of-magnitude lower final error than first-order methods (Adam, SGD) and quasi-Newton methods, and – crucially – enables natural-gradient training of PINNs at this scale on a single GPU.

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