Hydrodynamic Simulations of the Sunyaev‐Zeldovich Effect(s)
Author(s) -
Volker Springel,
Martin White,
Lars Hernquist
Publication year - 2001
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/319473
Subject(s) - cosmic microwave background , physics , astrophysics , redshift , reionization , adiabatic process , kinetic energy , anisotropy , spectral density , amplitude , angular diameter , matter power spectrum , thermal , computational physics , galaxy , classical mechanics , optics , quantum mechanics , stars , statistics , mathematics , meteorology
We have performed a sequence of high resolution hydrodynamic simulations ofstructure formation in a LCDM model to study the thermal and kineticSunyaev-Zel'dovich (SZ) effects. Including only adiabatic gas physics, wedemonstrate that our simulations for the thermal effect are converged down tosub-arcminute scales. In this model, the angular power spectrum of CMBanisotropies induced by the thermal effect peaks at l~10^4, and reaches anamplitude just below current observational upper limits. Fluctuations due tothe kinetic effect are a factor of ~30 lower in power and peak at slightlysmaller angular scales. We identify individual SZ sources and compute theircounts as a function of source strength and angular size. We present apreliminary investigation of the consequences of an early epoch of energyinjection which tends to suppress power on small angular scales, while givingrise to additional power on largescales from the reheated IGM at high redshift.
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