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The Physics of Microwave Background Anisotropies

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arxiv astro-ph/9504057 v1 pith:TKJXUDQR submitted 1995-04-18 astro-ph

Wayne Hu , Naoshi Sugiyama , Joseph Silk This is my paper
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keywords anisotropiesbackgrounddynamicsformationmicrowavestructureamountanisotropy
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Cosmic microwave background anisotropies provide a vast amount of information on both structure formation in the universe and the background dynamics and geometry. The full physical content and detailed structure of anisotropies can be understood in a simple and intuitive fashion through a systematic investigation of the individual mechanisms for anisotropy formation, based on elementary gravitational and fluid dynamics.

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Cited by 1 Pith paper

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

  1. The Squealer: Sensification of model exploration and model misfit

    physics.data-an 2026-06 unverdicted novelty 7.0 of 10

    Introduces an auditory feedback tool called The Squealer that produces louder and more unpleasant squeals as model-data discrepancy increases during interactive curve adjustment.

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