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The Cosmic Microwave Background Radiation

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arxiv astro-ph/0002044 v1 pith:VRSZMUKQ submitted 2000-02-02 astro-ph

classification astro-ph
keywords backgroundcosmicmicrowaveradiationtheoreticalanisotropiesanisotropyassociated
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We summarize the theoretical and observational status of the study of the Cosmic Microwave Background radiation. Its thermodynamic spectrum is a robust prediction of the Hot Big Bang cosmology and has been confirmed observationally. There are now 76 observations of Cosmic Microwave Background anisotropy, which we present in a table with references. We discuss the theoretical origins of these anisotropies and explain the standard jargon associated with their observation.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Towards a multi-tracer neutrino mass measurement with line-intensity mapping

    astro-ph.CO 2024-12 conditional novelty 6.0 of 10

    AtLAST [CII] line-intensity mapping, combined with CMB-S4 and DESI BAO forecasts, could reach sigma(sum m_nu) ~ 18 meV, and ~11.5 meV with a 21-cm tau prior.

  2. Spontaneous scalarization around a black hole in a dark matter halo

    gr-qc 2026-07 reject novelty 4.0 of 10

    A Hernquist dark-matter halo is claimed to scalarize a central black hole, with the coupling quantized as η_n = −(n+1/2)²π³/(2C), but the mechanism requires ρ−p>0 while the paper's own formulas give ρ−p<0.

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