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New uniform diameter bounds in pro- groups
We give new upper bounds for the diameters of finite groups which do not depend on a choice of generating set. Our method exploits the commutator structure of certain profinite groups, in a fashion analogous to the Solovay–Kitaev procedure from quantum computation. We obtain polylogarithmic upper bounds for the diameters of finite quotients of groups with an analytic structure over a pro-p domain (with exponent depending on the dimension); Chevalley groups over a pro-p domain (with exponent independent of the dimension) and the Nottingham group of a finite field. We also discuss some consequences of our results for random walks on groups
Local permutation stability
We introduce a notion of "local stability in permutations" for finitely
generated groups. If a group is sofic and locally stable in our sense, then it
is also locally embeddable into finite groups (LEF). Our notion is weaker than
the "permutation stability" introduced by Glebsky-Rivera and
Arzhantseva-Paunescu, which allows one to upgrade soficity to residual
finiteness. We prove a necessary and sufficient condition for an amenable group
to be locally permutation stable, in terms of invariant random subgroups
(IRSs), inspired by a similar criterion for permutation stability due to
Becker, Lubotzky and Thom. We apply our criterion to prove that derived
subgroups of topological full groups of Cantor minimal subshifts are locally
stable, using Zheng's classification of IRSs for these groups. This last result
provides continuum-many groups which are locally stable, but not stable.Comment: 33 pages, comments welcome
Cool Core Bias in Sunyaev-Zel'dovich Galaxy Cluster Surveys
Sunyaev-Zeldovich (SZ) surveys find massive clusters of galaxies by measuring
the inverse Compton scattering of cosmic microwave background off of
intra-cluster gas. The cluster selection function from such surveys is expected
to be nearly independent of redshift and cluster astrophysics. In this work, we
estimate the effect on the observed SZ signal of centrally-peaked gas density
profiles (cool cores) and radio emission from the brightest cluster galaxy
(BCG) by creating mock observations of a sample of clusters that span the
observed range of classical cooling rates and radio luminosities. For each
cluster, we make simulated SZ observations by the South Pole Telescope and
characterize the cluster selection function, but note that our results are
broadly applicable to other SZ surveys. We find that the inclusion of a cool
core can cause a change in the measured SPT significance of a cluster between
0.01% - 10% at z > 0.3, increasing with cuspiness of the cool core and angular
size on the sky of the cluster (i.e., decreasing redshift, increasing mass). We
provide quantitative estimates of the bias in the SZ signal as a function of a
gas density cuspiness parameter, redshift, mass, and the 1.4 GHz radio
luminosity of the central AGN. Based on this work, we estimate that, for the
Phoenix cluster (one of the strongest cool cores known), the presence of a cool
core is biasing the SZ significance high by ~ 6%. The ubiquity of radio
galaxies at the centers of cool core clusters will offset the cool core bias to
varying degrees.Comment: 8 pages, 4 figures, accepted to Ap
Short Laws for Finite Groups of Lie Type
We produce new short laws in two variables valid in finite groups of Lie
type. Our result improves upon results of Kozma and the second named author,
and is sharp up to logarithmic factors, for all families except possibly the
Suzuki groups. We also produce short laws valid for generating pairs and random
pairs in finite groups of Lie type, and, conditional on Babai's diameter
conjecture, make effective the dependence of our bounds on the rank. Our proof
uses, among other tools, the Classification of Finite Simple Groups,
Aschbacher's structure theorem for maximal subgroups for classical groups, and
upper bounds on the diameters of finite simple groups due to Breuillard, Green,
Guralnick, Pyber, Szabo and Tao.Comment: 38 pages, comments welcom
Short laws for finite groups and residual finiteness growth
We prove that for every
n
∈
N
n \in \mathbb {N}
and
δ
>
0
\delta >0
there exists a word
w
n
∈
F
2
w_n \in F_2
of length
O
(
n
2
/
3
log
(
n
)
3
+
δ
)
O(n^{2/3} \log (n)^{3+\delta })
which is a law for every finite group of order at most
n
n
. This improves upon the main result of Andreas Thom [Israel J. Math. 219 (2017), pp. 469–478] by the second named author. As an application we prove a new lower bound on the residual finiteness growth of non-abelian free groups.</p
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