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Present and Future of the Cosmic Microwave Background pp 188–207Cite as

Microwave background anisotropies: Future plans

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Part of the book series: Lecture Notes in Physics ((LNP,volume 429))

Abstract

The role of CBR Anisotropies in Cosmology is briefly discussed. The various possible sources of noise and distortions -are analyzed. In particular we consider the effects of the elastic Thomson scattering between Cosmic Back ground Radiation (CBR) and primordial molecules, like H 2, H +2 , HeH +, HD, HD +, LiH, LiH +: primary CBR anisotropies are erased or attenuated for angular scales ≤ 10° ⇔ 50° and frequencies v ≤ 50 GHz.

Future space programs are illustrated.

Subject headings: Cosmology- Cosmic Background Anisotropies- Post-Recombination Universe

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Authors and Affiliations

  1. Laboratoire de Radiastronomie Millimetrique, Observatoire de Meudon, Unité CNRS-336, 5, Place Jules Janssen, 92195, MEUDON Cédex, FRANCE

    Roberto Maoli

  2. IFA-CNR Pzle L. Sturzo 31, Rome, Italy

    Bianca Melchiorri

  3. Ecole Normale Superieure, 24 Rue Lhomond, F-75231, PARIS Cédex 0.5, FRANCE

    Monique Signore

  4. Department of Physics Guglielmo Marconi, University of Rome “La Sapienza”, Pzle Aldo Moro 2, ROME, Italy

    Paolo de Bernardis, Silvia Masi, Francesco Melchiorri & Danilo Tosti

Authors
  1. Paolo de Bernardis
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  2. Roberto Maoli
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  3. Silvia Masi
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  4. Bianca Melchiorri
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  5. Francesco Melchiorri
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  6. Monique Signore
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  7. Danilo Tosti
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Editor information

José Luis Sanz Enrique Martínez-González Laura Cayón

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© 1994 Springer-Verlag

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de Bernardis, P. et al. (1994). Microwave background anisotropies: Future plans. In: Sanz, J.L., Martínez-González, E., Cayón, L. (eds) Present and Future of the Cosmic Microwave Background. Lecture Notes in Physics, vol 429. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-57755-6_47

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  • DOI: https://doi.org/10.1007/3-540-57755-6_47

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-57755-3

  • Online ISBN: 978-3-540-48328-1

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