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- W2040378964 abstract "This Letter explores the influences of intracluster magnetic fields (1 μG) submerged in the hot electron gas on the classic Sunyaev-Zel'dovich effect (SZE) and on the thermal bremsstrahlung in X-ray emissions. As the Larmor frequency is much higher than all collision frequencies, the presence of a magnetic field may lead to an anisotropic velocity distribution of hot electrons. For the two-temperature relativistic Maxwell-Boltzmann distribution, we compute modifications to the classical thermal SZE. Intracluster magnetic fields tend to enhance the SZE with steeper radial variations, which bear important consequences for cluster-based estimates of cosmological parameters. By applying the magnetic SZE theory to spectral observations of SZE and Chandra X-ray emissions from the galaxy cluster A2163, a ~30-40 μG central core magnetic field B0 is predicted. For the SZE and Chandra X-ray spectral observations of the Coma Cluster, our theoretical analysis is also consistent with an observationally inferred B0 10 μG. As the magnetic SZE is redshift (z) independent, this mechanism might offer a potentially important and unique way of probing intracluster magnetic fields in the expanding universe." @default.
- W2040378964 created "2016-06-24" @default.
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- W2040378964 date "2004-04-01" @default.
- W2040378964 modified "2023-09-27" @default.
- W2040378964 title "Magnetic Sunyaev-Zel'dovich Effect in Galaxy Clusters" @default.
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- W2040378964 doi "https://doi.org/10.1086/420896" @default.
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