We introduce a semi-parametric method to simultaneously infer both the drift and volatility functions of a discretely observed scalar diffusion. We introduce spline bases to represent these functions and develop a Markov chain Monte Carlo algorithm to infer, a posteriori, the coefficients of these functions in the spline basis. A key innovation is that we use spline bases to model transformed versions of the drift and volatility functions rather than the functions themselves. The output of the algorithm is a posterior sample of plausible drift and volatility functions that are not constrained to any particular parametric family. The flexibility of this approach provides practitioners a powerful investigative tool, allowing them to posit parametric models to better capture the underlying dynamics of their processes of interest. We illustrate the versatility of our method by applying it to challenging datasets from finance, paleoclimatology, and astrophysics. In view of the parametric diffusion models widely employed in the literature for those examples, some of our results are surprising since they call into question some aspects of these models.
翻译:我们引入了半参数方法,以同时推算离散观测的星标扩散的漂移和挥发功能。我们引入了样条基以代表这些功能,并开发了Markov链 Monte Carlo 算法,以推断这些函数在样条基中的系数。一个关键的创新是,我们使用样条基来模拟漂移和挥发功能的转变版本,而不是功能本身。算法的输出是不受任何特定参数组制约的表面漂移和挥发功能的样板。这一方法的灵活性为从业人员提供了一个强大的调查工具,使他们能够假设参数模型,以更好地捕捉他们感兴趣的过程的基本动态。我们用它来对金融、古气候学和天体物理学的数据集提出挑战,以此来说明我们的方法的多功能。鉴于文献中为这些实例广泛使用的参数扩散模型,我们的一些结果令人吃惊,因为它们质疑了这些模型的某些方面。