1995/05/31 by Andreas Albrecht, David Coulson, Pedro G. Ferreira +3 · 134 citations
Physics and Astronomy · #Anisotropy #Astrophysics #Causality (physics) #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Inflation (cosmology) #Microwave #Physics #Planck #Quantum mechanics #Radio Astronomy Observations and Technology #Randomness #Statistical physics #Statistics #Theoretical physics #astro-ph
paper · pdf · doi:10.1103/physrevlett.76.1413
published in Physical Review Letters 76(9), 1413-1416 (American Physical Society) · uuencoded tex file and 4 postscript figure files, 8 pages. Also available at http://euclid.tp.ph/Papers/index.html; Changes: Minor changes reflect final published version
openalex publication_date 1996/02/26 · arxiv created 1996/02/29 · arxiv updated 2010/04/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Fluctuations in the cosmic microwave background (CMB) temperature are being studied with ever increasing precision. Two competing types of theories might describe the origins of these fluctuations: ``inflation'' and ``defects.'' Here we show how the differences between these two scenarios can give rise to striking signatures in the microwave fluctuations on small scales, assuming a standard recombination history. These should enable high resolution measurements of CMB anisotropies to distinguish between these two broad classes of theories, independent of the precise details of each.