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Asymptotic expansion of the expected Minkowski functional for isotropic central limit random fields

Published online by Cambridge University Press:  14 July 2023

Satoshi Kuriki*
Affiliation:
The Institute of Statistical Mathematics
Takahiko Matsubara*
Affiliation:
High Energy Accelerator Research Organization (KEK)
*
*Postal address: The Institute of Statistical Mathematics, 10-3 Midoricho, Tachikawa, Tokyo 190-8562, Japan. Email address: kuriki@ism.ac.jp
**Postal address: Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Oho 1-1, Tsukuba, Ibaraki 305-0801, Japan. Email address: tmats@post.kek.jp

Abstract

The Minkowski functionals, including the Euler characteristic statistics, are standard tools for morphological analysis in cosmology. Motivated by cosmic research, we examine the Minkowski functional of the excursion set for an isotropic central limit random field, whose k-point correlation functions (kth-order cumulants) have the same structure as that assumed in cosmic research. Using 3- and 4-point correlation functions, we derive the asymptotic expansions of the Euler characteristic density, which is the building block of the Minkowski functional. The resulting formula reveals the types of non-Gaussianity that cannot be captured by the Minkowski functionals. As an example, we consider an isotropic chi-squared random field and confirm that the asymptotic expansion accurately approximates the true Euler characteristic density.

Type
Original Article
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of Applied Probability Trust

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References

Adler, R. J. (1981). The Geometry of Random Fields. John Wiley, Chichester.Google Scholar
Adler, R. J. and Taylor, J. E. (2007). Random Fields and Geometry. Springer, New York.Google Scholar
Adler, R. J. and Taylor, J. E. (2011). Topological Complexity of Smooth Random Functions. Springer, Heidelberg.Google Scholar
Bhattacharya, R. N. and Rao, R. R. (2010). Normal Approximation and Asymptotic Expansions. Society for Industrial and Applied Mathematics, Philadelphia.Google Scholar
Chamandy, N., Worsley, K. J., Taylor, J. and Gosselin, F. (2008). Tilted Euler characteristic densities for central limit random fields, with application to ‘bubbles’. Ann. Statist. 36, 24712507.Google Scholar
Cheng, D. and Schwartzman, A. (2018). Expected number and height distribution of critical points of smooth isotropic Gaussian random fields. Bernoulli 24, 34223446.Google Scholar
Davis, A. W. (1980). Invariant polynomials with two matrix arguments, extending the zonal polynomials. In Multivariate Analysis V: Proceedings of the Fifth International Symposium on Multivariate Analysis, North-Holland, Amsterdam, pp. 287–299.Google Scholar
Fantaye, Y., Marinucci, D., Hansen, F. and Maino, D. (2015). Applications of the Gaussian kinematic formula to CMB data analysis. Phys. Rev. D 91, article no. 063501.Google Scholar
Hikage, C., Komatsu, E. and Matsubara, T. (2006). Primordial non-Gaussianity and analytical formula for Minkowski functionals of the cosmic microwave background and large-scale structure. Astrophys. J. 653, 1126.CrossRefGoogle Scholar
Hug, D. and Schneider, R. (2002). Kinematic and Crofton formulae of integral geometry: recent variants and extensions. In Homenatge al Professor Llus Santaló i Sors, ed. C. Barceló i Vidal, Universitat de Girona, pp. 51–80.Google Scholar
Kuriki, S., Takemura, A. and Taylor, J. E. (2022). The volume-of-tube method for Gaussian random fields with inhomogeneous variance. J. Multivariate Anal. 188, article no. 104819, 23 pp.Google Scholar
Marinucci, D. and Peccati, G. (2011). Random Fields on the Sphere: Representation, Limit Theorems and Cosmological Applications. Cambridge University Press.Google Scholar
Matsubara, T. (2003). Statistics of smoothed cosmic fields in perturbation theory. I. Formulation and useful formulae in second-order perturbation theory. Astrophys. J. 584, 133.Google Scholar
Matsubara, T. (2010). Analytic Minkowski functionals of the cosmic microwave background: second-order non-Gaussianity with bispectrum and trispectrum. Phys. Rev. D 81, article no. 083505.Google Scholar
Matsubara, T. and Kuriki, S. (2021). Weakly non-gaussian formula for the minkowski functionals in general dimensions. Phys. Rev. D 104, 103522.Google Scholar
Matsubara, T. and Yokoyama, J. (1996). Genus statistics of the large-scale structure with non-Gaussian density fields. Astrophys. J. 463, 409419.Google Scholar
McCullagh, P. (1987). Tensor Methods in Statistics. Chapman and Hall, London.Google Scholar
Panigrahi, S., Taylor, J. and Vadlamani, S. (2019). Kinematic formula for heterogeneous Gaussian related fields. Stoch. Process. Appl. 129, 24372465.Google Scholar
Collaboration, Planck (2014). Planck 2013 results. XXIV. Constraints on primordial non-Gaussianity. A&A 571, article no. A24, 58 pp.Google Scholar
Pranav, P. et al. (2019). Topology and geometry of Gaussian random fields I: on Betti numbers, Euler characteristic, and Minkowski functionals. Monthly Notices R. Astronom. Soc. 485, 41674208.Google Scholar
Schmalzing, J. and Buchert, T. (1997). Beyond genus statistics: a unifying approach to the morphology of cosmic structure. Astrophys. J. 482, L1L4.Google Scholar
Schmalzing, J. and Górski, K. M. (1998). Minkowski functionals used in the morphological analysis of cosmic microwave background anisotropy maps. Monthly Notices R. Astronom. Soc. 297, 355365.CrossRefGoogle Scholar
Schneider, R. and Weil, W. (2008). Stochastic and Integral Geometry. Springer, Berlin.Google Scholar
Takemura, A. and Kuriki, S. (2002). On the equivalence of the tube and Euler characteristic methods for the distribution of the maximum of Gaussian fields over piecewise smooth domains. Ann. Appl. Prob. 12, 768796.Google Scholar
Taylor, J. E. (2006). A Gaussian kinematic formula. Ann. Prob. 34, 122158.Google Scholar
Tomita, H. (1986). Curvature invariants of random interface generated by Gaussian fields. Progress Theoret. Phys. 76, 952955.Google Scholar
Worsley, K. J. (1994). Local maxima and the expected Euler characteristic of excursion sets of $\chi^{2}$ and t fields. Adv. Appl. Prob. 26, 1342.Google Scholar
Worsley, K. J. (1995). Boundary corrections for the expected Euler characteristic of excursion sets of random fields, with an application to astrophysics. Adv. Appl. Prob. 27, 943959.Google Scholar