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Speedy Sound and Cosmic Structure

2008/03/31 by João Magueijo, Joao Magueijo · 4 citations
Mathematics · Physics and Astronomy · #Acoustics #Astrophysics #Black Holes and Theoretical Physics #COSMIC cancer database #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Heuristics #Mathematics #Mechanism (biology) #Physics #Quantum mechanics #Scalar (mathematics) #Speed of sound #Statistical physics #Theoretical physics #Universe #astro-ph #gr-qc #hep-ph

paper · pdf · doi:10.1103/physrevlett.100.231302

published as Phys.Rev.Lett.100:231302,2008 · To be published in Phys. Rev. Letters

arxiv created 2008/06/04 · openalex publication_date 2008/06/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

If the speed of sound were vastly larger in the early Universe, a near scale-invariant spectrum of density fluctuations could have been produced even if the Universe did not submit to conventional solutions to the horizon problem. We examine how the mechanism works, presenting full mathematical solutions and their heuristics. We then discuss several concrete models based on scalar fields and hydrodynamical matter that realize this mechanism, but stress that the proposed mechanism is more fundamental and general.

Citations

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