Telescopic growth conjecture for finite type h spectra

Let XX be a finite spectrum of type hh, and let ϖT(h)(X,n)\varpi_{\mathrm{T}(h)}(X,n) denote the size function measuring its telescopic homotopy groups through degree nn. Telescopic growth conjecture. The telescopic homotopy groups satisfy

log(ϖT(h)(X,n))=(h2)log(n)+O(1).\log\left(\varpi_{\mathrm{T}(h)}(X,n)\right)=\binom{h}{2}\log(n)+O(1).

This conjecture is motivated by the calculation for the non-finite spectrum y(h)y(h) and Morita invariance of size functions; it predicts the growth for every compact type hh spectrum while accounting for the extra polynomial generators present in y(h)y(h).

Sources & referencesView supporting material

Primary source

Robert Burklund and Andrew Senger, “How Big are the Stable Homotopy Groups of Spheres?”, arXiv:2203.00670 (2022).

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