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Bingyuan Wei

Publications and source records attributed to Bingyuan Wei.

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Higher-order Diffusion Sampling via Chebyshev Interpolation and Gauss--Seidel Iterations

Higher-order ODE solvers have shown strong empirical promise for accelerating diffusion models through the probability flow ODE, but rigorous non-asymptotic guarantees for such acceleration remain limited. In this paper, we develop a Chebyshev--Gauss--Seidel higher-order sampler and establish a non-asymptotic convergence guarantee that allows the approximation order to grow logarithmically with the number of outer iterations. In the exact-score setting, up to logarithmic factors, the proposed sampler requires at most \[ d^{1+o_T(1)}\varepsilon^{-1/K_1} \] score functions to approximate the target distribution on \(\mathbb{R}^d\) within total variation distance \(\varepsilon\), where \(o_T(1)\to 0\) as \(T\to\infty\) and \(K_1>0\) is a sufficiently large constant. The analysis assumes only a polynomial second-moment bound on the target distribution, thereby relaxing the bounded-support condition imposed in existing higher-order theory. Moreover, the guarantee is robust to score and Jacobian estimation errors and does not require higher-order smoothness assumptions on the score estimates. Numerical experiments on anisotropic Gaussian mixture benchmarks support the predicted improvement in the accuracy--cost tradeoff under finite score-evaluation budgets.

math.NA

Quasinormal Modes of Bardeen Black Hole in 5-dimensional Gauss-Bonnet Gravity

This study addressed the scalar field quasinormal ringing behavior of black holes. We investigated scalar field perturbations in Bardeen black hole spacetime in 5-dimensional Einstein-Gauss-Bonnet (EGB) gravity. Using the 3rd-order WKB approximation and the finite-difference method, we computed the frequency of quasinormal modes (QNMs) in the spacetime background. The calculations demonstrated that the real part of the QNMs $ω$ increased, whereas the imaginary part decreased with increase in the magnetic charge parameter $Q$ of the Bardeen black hole for a fixed Gauss-Bonnet parameter $α$. This was also valid when $Q$ was fixed and $α$ increased; where in the real part of the QNMs increased and the absolute value of the imaginary part decreased. However, the change in the latter case was more significant than that in the former; thus, the frequency of eigenvibration of this black hole background under the scalar field perturbation increased and the decay of eigenvibration decreased with increase in $α$ or $Q^2$. Moreover, this result shows that the effect of $α$ on the intrinsic vibration of this black hole was greater than that of $Q $.Finally we found an interesting phenomenon by comparing black holes in 4 and 5 dimensions. With higher dimensions, the real part of the QNMs changes more obviously, but the imaginary part of the QNMs is almost unchanged. This phenomenon also indicates that the frequency of gravitational waves released by higher dimensional black holes becomes larger, but the decay rate is almost constant.

hep-th