Telescopic growth conjecture for finite type h spectra

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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).

References

Primary source

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

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