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Adiabatic CMB perturbations in pre-Big-Bang string cosmology

2001/09/30 by Kari Enqvist, Martin S. Sloth · 880 citations
Physics and Astronomy · #Adiabatic process #Astrophysics #Axion #Big Bang (financial markets) #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Inflation (cosmology) #Instanton #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum electrodynamics #Quantum mechanics #String (physics) #Theoretical physics #Universe #astro-ph #hep-ph #hep-th

paper · pdf · doi:10.1016/s0550-3213(02)00043-3

published in Nuclear Physics B 626(1-2), 395-409 (Elsevier BV) · 15 pages, 1 figure; Version to appear in Nucl.Phys.B. Figure improved, discussion and one reference added

arxiv created 2002/01/30 · openalex publication_date 2002/04/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

We consider the pre-big bang scenario with a massive axion field which starts to dominate energy density when oscillating in an instanton-induced potential and subsequently reheats the universe as it decays into photons, thus creating adiabatic CMB perturbations. We find that the fluctuations in the axion field can give rise to a nearly flat spectrum of adiabatic perturbations with a spectral tilt Δn in the range -0.1 \lesssim Δn \lesssim 1.

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