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ΔT/T beyond linear theory

  • Enrique Martínez-González
Part III The Cosmic Microwave Background
Part of the Lecture Notes in Physics book series (LNP, volume 470)

Abstract

The major contribution to the anisotropy of the temperature of the Cosmic Microwave Background (CMB) radiation is believed to come from the interaction of linear density perturbations with the radiation previous to the decoupling time. Assuming a standard thermal history for the gas after recombination, only the gravitational field produced by the linear density perturbations present on a Ω≠1 universe can generate anisotropies at low z (these anisotropies would manifest on large angular scales). However, secondary anisotropies are inevitably produced during the nonlinear evolution of matter at late times even in a universe with a standard thermal history. Two effects associated to this nonlinear phase can give rise to new anisotropies: the time-varying gravitational potential of nonlinear structures (Rees-Sciama RS effect) and the inverse Compton scattering of the microwave photons with hot electrons in clusters of galaxies (Sunyaev-Zeldovich SZ effect). These two effects can produce distinct imprints on the CMB temperature anisotropy. We discuss the amplitude of the anisotropies expected and the relevant angular scales in different cosmological scenarios. Future sensitive experiments will be able to probe the CMB anisotropies beyong the first order primary contribution.

Keywords

Cosmic Microwave Background Cosmic Microwave Background Anisotropy Rich Cluster Microwave Photon Inverse Compton Scattering 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1996

Authors and Affiliations

  • Enrique Martínez-González
    • 1
  1. 1.Instituto de Física de Cantabria, Consejo Superior de InvestigacionesCientíficas-Universidad de Cantabria, Facultad de CienciasSantanderSpain

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