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Polarization Signatures of Clusters in the Microwave Background

Published online by Cambridge University Press:  26 May 2016

Anthony. Challinor*
Affiliation:
Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE, UK

Abstract

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Compton scattering of photons from ionised gas in galaxy clusters along the line of sight leaves an imprint in the polarization of the cosmic microwave background. We investigate this process taking account of the effects of relativistic electron velocity dispersion and primordial anisotropy on the frequency spectrum of the generated polarization. We also discuss the prospects of detecting such effects with the Planck survey.

Type
Part XII: Poster Papers
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Challinor, A. D., Ford, M. T. & Lasenby, A. N. 2000, MNRAS, 312, 159.Google Scholar
Sazonov, S. Y. & Sunyaev, R. A. 1999, MNRAS, 310, 765.Google Scholar
Sunyaev, R. A. & Zel'dovich, Y. B. 1980, MNRAS, 190, 413.Google Scholar
Zel'dovich, Y. B. & Sunyaev, R. A. 1980, Astron. Lett., 6, 285.Google Scholar