Hole probability for zeroes of Gaussian Taylor series with finite radii of convergence

Jeremiah Buckley*, Alon Nishry, Ron Peled, Mikhail Sodin

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

We study a family of random Taylor series F(z)=∑n≥0ζnanznwith radius of convergence almost surely 1 and independent, identically distributed complex Gaussian coefficients (ζn) ; these Taylor series are distinguished by the invariance of their zero sets with respect to isometries of the unit disk. We find reasonably tight upper and lower bounds on the probability that F does not vanish in the disk { | z| ⩽ r} as r↑ 1. Our bounds take different forms according to whether the non-random coefficients (an) grow, decay or remain of the same order. The results apply more generally to a class of Gaussian Taylor series whose coefficients (an) display power-law behavior.

Original languageEnglish
Pages (from-to)377-430
Number of pages54
JournalProbability Theory and Related Fields
Volume171
Issue number1-2
DOIs
StatePublished - 1 Jun 2018

Funding

FundersFunder number
Seventh Framework Programme335141
European Commission
Israel Science Foundation166/11, 382/15, 1048/11, 861/15

    Keywords

    • 30B20
    • 30C15
    • 60G55

    Fingerprint

    Dive into the research topics of 'Hole probability for zeroes of Gaussian Taylor series with finite radii of convergence'. Together they form a unique fingerprint.

    Cite this