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Journal ArticleDOI

Spectrum of the Sunyaev-Zel'dovich effect for high electron temperatures

R. Fabbri
- 01 Jul 1981 - 
- Vol. 77, Iss: 2, pp 529-537
TLDR
In this article, the spectral shape of the Sunyaev-Zel'dovich effect in the cosmic background radiation was analyzed in detail, taking into account relativistic corrections for a hot electron gas.
Abstract
We analyse in detail the spectral shape of the Sunyaev-Zel'dovich effect in the cosmic background radiation, taking into account the relativistic corrections for a hot electron gas We calculate the displacement of the zero-signal frequency, which is especially informative in a new method for measuring the millimetric temperature of the background radiation; we also present a simple analytical expression, to be used to fit the experimental data in spectral measurements of the effect in very hot cluster gases

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Citations
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Journal ArticleDOI

The Sunyaev-Zel’dovich Effect

TL;DR: The Sunyaev-Zel-dovich effect as mentioned in this paper causes a change in the apparent brightness of the cosmic microwave background radiation towards a cluster of galaxies or any other reservoir of hot plasma.
Journal ArticleDOI

Cosmology with the Sunyaev-Zel'dovich Effect

TL;DR: The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-scale structure of the universe as traced by massive clusters of galaxies as mentioned in this paper.

The Sunyaev-Zel'dovich effect *

TL;DR: The Sunyaev-Zel-dovich effect as discussed by the authors causes a change in the apparent brightness of the cosmic microwave background radiation towards a cluster of galaxies or any other reservoir of hot plasma.
Journal ArticleDOI

Relativistic Corrections to the Sunyaev-Zeldovich Effect

TL;DR: In this article, an extension of the Kompaneets equation which allows relativistic effects to be included to any desired order is presented, which is expected to be very accurate over all regions of the cosmic microwave background spectrum for kBTe up to ~10 keV.
Journal ArticleDOI

The Cosmic Microwave Background

TL;DR: Current CMB data is used to set some preliminary constraints on the values of fundamental cosmological parameters Ω and Ho using the maximum likelihood technique and secondary anisotropies due to the Sunyaev-Zel’dovich effect are described.
References
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Journal ArticleDOI

The interaction of matter and radiation in a hot-model universe

TL;DR: In this article, it was shown that any injection of energy att>1010 sec (red shiftz <105) leads to deviation from an equilibrium spectrum, and that a period of neutral hydrogen in the evolution of the universe is unavoidable.
Journal ArticleDOI

Small-scale fluctuations of relic radiation*

TL;DR: In this paper, it is shown that an adiabatic connection exists between the density perturbations at the moment of recombination of the initial plasma and fluctuations of the observed temperature of radiation δT/T=δϱm/3ϱ m.
Journal ArticleDOI

Distortion of the microwave background by a hot intergalactic medium

TL;DR: In this article, the distortion of the cosmic microwave background by a hot, optically thin intergalactic medium (IGM) is calculated using the full frequency redistribution function, and it is shown that even if the IGM produces all the cosmic X-ray background, it is not detectable in the present observational data.
Journal ArticleDOI

The determination of q sub 0 using X-ray and microwave observations of galaxy clusters

TL;DR: In this article, X-ray and microwave observations of the hot gas in a rich cluster of galaxies can be combined to give a direct and model-free measurement of the angular diameter distance to the cluster.
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