Relativistic SZ temperatures and hydrostatic mass bias for massive clusters in the FLAMINGO simulations
arxiv(2024)
摘要
The relativistic Sunyaev-Zel'dovich (SZ) effect can be used to measure
intracluster gas temperatures independently of X-ray spectroscopy. Here, we use
the large-volume FLAMINGO simulation suite to determine whether SZ y-weighted
temperatures lead to more accurate hydrostatic mass estimates in massive
(M_ 500c > 7.5× 10^14 M_⊙) clusters than when using
X-ray spectroscopic-like temperatures. We find this to be the case, on average.
The median bias in the SZ mass at redshift zero is < b > ≡
1-< M_ 500c,hse/M_ 500c,true> = -0.05 ± 0.01, over 4
times smaller in magnitude than the X-ray spectroscopic-like case, < b
> = 0.22 ± 0.01. However, the scatter in the SZ bias, σ_b≈ 0.2, is around 40 per cent larger than for the X-ray case. We show
that this difference is strongly affected by clusters with large pressure
fluctuations, as expected from shocks in ongoing mergers. Selecting the
clusters with the best-fitting generalized NFW pressure profiles, the median SZ
bias almost vanishes, < b > = -0.009 ± 0.005, and the scatter is
halved to σ_b≈ 0.1. We study the origin of the SZ/X-ray
difference and find that, at R_ 500c and in the outskirts, SZ weighted
gas better reflects the hot, hydrostatic atmosphere than the X-ray weighted
gas. The SZ/X-ray temperature ratio increases with radius, a result we find to
be insensitive to variations in baryonic physics, cosmology and numerical
resolution.
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