The geometrical meaning of statistical isotropy of smooth random fields in two dimensions
arXiv:2109.05726 · doi:10.1103/PhysRevD.104.123516
Abstract
We revisit the geometrical meaning of statistical isotropy that is manifest in excursion sets of smooth random fields in two dimensions. Using the contour Minkowski tensor, $\W_1$, as our basic tool we first examine geometrical properties of single structures. For simple closed curves in two dimensions we show that $\W_1$ is proportional to the identity matrix if the curve has -fold symmetry, with . Then we elaborate on how $\W_1$ maps any arbitrary shaped simple closed curve to an ellipse that is unique up to translations of its centroid. We also carry out a comparison of the shape parameters, and , defined using $\W_1$, with the filamentarity parameter defined using two scalar Minkowski functionals - area and contour length. We show that they contain complementary shape information, with $\W_1$ containing additional information of orientation of structures. Next, we apply our method to boundaries of excursion sets of random fields and examine what statistical isotropy means for the geometry of the excursion sets. Focusing on Gaussian isotropic fields, and using a semi-numerical approach we quantify the effect of finite sampling of the field on the geometry of the excursion sets. In doing so we obtain an analytic expression for which takes into account the effect of finite sampling. Finally we derive an analytic expression for the ensemble expectation of $\W_1$ for Gaussian anisotropic random fields. Our results provide insights that are useful for designing tests of statistical isotropy using cosmological data.
14 pages
References in corpus (6)
- Tensor Minkowski Functionals for random fields on the sphere
- Tracking down the origin of superbubbles and supergiant shells in the Magellanic Clouds with Minkowski tensor analysis
- The nature of non-Gaussianity and statistical isotropy of the 408 MHz Haslam synchrotron map
- Application of Contour Minkowski Tensor and Statistic to the Planck -mode data
- Morphology of CMB fields -- effect of weak gravitational lensing
- Local patch analysis for testing statistical isotropy of the Planck convergence map
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