2001/10/31 by Richard Easther, Brian R. Greene, Brian Greene +2 · 4 citations
Mathematics · Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Inflation (cosmology) #Mathematics #Observable #Particle physics #Perturbation (astronomy) #Perturbation theory (quantum mechanics) #Physics #Power law #Quantum mechanics #Spectral density #Spectrum (functional analysis) #Statistical physics #Statistics #Theoretical physics #astro-ph #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.67.063508
published as Phys.Rev. D67 (2003) 063508 · Revtex 4, 3 eps figs, 4 pages
arxiv created 2002/04/16 · openalex publication_date 2003/03/26 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We analyze the impact of certain modifications to short distance physics on the inflationary perturbation spectrum. For the specific case of power-law inflation, we find distinctive---and possibly observable---effects on the spectrum of density perturbations.