MarkTechPost@AI 2024年07月03日
Gibbs Diffusion (GDiff): A New Bayesian Blind Denoising Method with Applications in Image Denoising and Cosmology
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Gibbs Diffusion (GDiff) 是一种新的贝叶斯盲去噪方法,它通过同时对噪声参数和信号参数进行后验采样来解决传统扩散模型去噪方法需要事先知道噪声水平和协方差的限制。GDiff 方法在图像去噪和宇宙学领域都有应用,例如可以用来恢复被彩色噪声模糊的图像,并同时估计噪声参数,以及在宇宙微波背景 (CMB) 数据处理中,通过对噪声参数进行贝叶斯推断来约束宇宙演化的模型。

🤔 **GDiff 的核心思想:** GDiff 通过将信号的先验分布映射到一系列噪声分布,然后使用蒙特卡罗采样来推断噪声参数,从而实现对噪声参数和信号参数的联合推断。 GDiff 方法利用了扩散模型的特性,将信号的先验分布映射到一系列噪声分布,并使用蒙特卡罗采样来推断噪声参数。这种方法的关键在于它能够同时对信号参数和噪声参数进行推断,从而克服了传统扩散模型去噪方法需要事先知道噪声水平和协方差的限制。

🔭 **GDiff 在图像去噪中的应用:** GDiff 方法可以用于恢复被彩色噪声模糊的图像,并同时估计噪声参数。它在盲去噪问题上取得了显著的效果,优于传统的基线方法。 GDiff 方法在图像去噪中的应用主要集中在盲去噪问题上,即在不知道噪声参数的情况下恢复图像。它通过同时对信号参数和噪声参数进行推断,能够有效地恢复被彩色噪声模糊的图像,并同时估计噪声参数。

🌌 **GDiff 在宇宙学中的应用:** GDiff 方法可以用来增强对宇宙模型的理解,通过对噪声参数进行贝叶斯推断来约束宇宙演化的模型。 GDiff 方法在宇宙学中的应用主要体现在对宇宙微波背景 (CMB) 数据的处理上。CMB 数据中包含了大量噪声,而 GDiff 方法可以通过对噪声参数进行贝叶斯推断,来约束宇宙演化的模型,从而增强对宇宙模型的理解。

🏆 **GDiff 的优势:** GDiff 方法克服了传统扩散模型去噪方法的局限性,能够在不知道噪声参数的情况下,更准确地恢复信号。 GDiff 方法克服了传统扩散模型去噪方法的局限性,能够在不知道噪声参数的情况下,更准确地恢复信号。它在图像去噪和宇宙学领域都有应用,并取得了显著的效果,为解决盲去噪问题提供了新的思路。

With the recent advancement of deep generative models, the challenge of denoising has also become apparent. Diffusion models are trained and designed similarly to denoisers, and their modeled distributions agree with denoising priors when applied in a Bayesian setting. However, blind denoising, when these parameters are unknown, is difficult since conventional diffusion-based denoising techniques require previous knowledge of the noise level and covariance.

In a recent study, a team of researchers from Ecole Polytechnique, Institut Polytechnique de Paris and Flatiron Institute proposed a unique approach called Gibbs Diffusion (GDiff) to overcome the limitations. This approach allows posterior sampling of the noise parameters in addition to the signal parameters simultaneously. The creation of a Gibbs method specifically designed for situations involving arbitrary parametric Gaussian noise is the main feature here. The two kinds of sample phases that the algorithm uses in alternation are as follows.

    Conditional Diffusion Model Sampling: In this stage, a trained diffusion model is used to map the signal’s previous distribution to a family of noise distributions. This model considers the noise’s peculiarities and helps in signal inference.
    Monte Carlo Sampling: Inferring the noise parameters is the main goal of the Monte Carlo Sampling stage. The approach can estimate the parameters that characterize the noise distribution by using a Monte Carlo sampler.

The team has shared that the theoretical evaluation of the Gibbs Diffusion method quantifies the flaws in the Gibbs stationary distribution resulting from the diffusion model. It also offers recommendations for diagnostic applications. Two applications have been highlighted to illustrate the effectiveness of this method.

    Blind Denoising of Natural Images: In this application, colored noise is used to blur images, but its amplitude and spectral index are unknown. The GDiff approach recovers the clean image and characterizes the noise at the same time, which allows it to successfully perform the blind denoising problem.
    Cosmology problem: The second application deals with data processing related to the cosmic microwave background (CMB). Within this framework, constraining models of the universe’s evolution are achieved through Bayesian inference of the noise parameters. The GDiff approach can be used to enhance comprehension of cosmological models by inferring the noise parameters.

The team has shared their primary contributions, which are as follows.

    To address the difficulties of modeling the prior distribution based on samples​ and sampling the posterior, the team has introduced Gibbs Diffusion (GDiff), a unique approach to blind denoising.
    The team has provided a solid theoretical framework for GDiff by establishing requirements for the presence of stationary distribution within the method and quantifying the propagation of inference mistakes.
    The effectiveness of the approach has been showcased in two domains: cosmology, where it supports the Bayesian inference of noise parameters to constrain models of the Universe’s evolution, and blind denoising of natural photos with arbitrary colored noise, where GDiff beats traditional baselines.

In conclusion, Gibbs Diffusion is a major breakthrough in denoising that makes it possible to recover signals more thoroughly and precisely in situations where noise parameters are unknown.


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The post Gibbs Diffusion (GDiff): A New Bayesian Blind Denoising Method with Applications in Image Denoising and Cosmology appeared first on MarkTechPost.

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Gibbs Diffusion 盲去噪 贝叶斯推断 图像去噪 宇宙学
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