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Seeding of primordial perturbations during a decelerated expansion

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

Abstract

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.

Citations

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