2006/09/30 by Yun-Song Piao · 4 citations
Mathematics · Physics and Astronomy · #Astronomy #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Field (mathematics) #Geometry #Mathematics #Metric expansion of space #Observable #Perturbation (astronomy) #Physics #Quantum mechanics #Scalar (mathematics) #Scalar field #Seeding #Theoretical physics #Thermodynamics #gr-qc
paper · pdf · doi:10.1103/physrevd.75.063517
published as Phys.Rev.D75:063517,2007 · 5 pages, 3 figures, more details and clarifications added, refs. added, new version with 6 pages has been splitted into various sections, to be published in PRD, v3, matched to published version
openalex publication_date 2007/03/26 · arxiv created 2007/05/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A scalar field with a modified dispersion relation may seed, under certain conditions, the primordial perturbations during a decelerated expansion. In this paper we examine whether and how these perturbations can be responsible for the structure formation of the observable universe. We discuss relevant difficulties and possible solutions.