1998/09/10 by Marie-Noëlle Célérier, M. N. Celerier, Jean Schneider +1 · 1 citation
Physics and Astronomy · #Astronomy #Big Bang (financial markets) #Big Bounce #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Dark energy #De Sitter universe #Economics #Galaxies: Formation, Evolution, Phenomena #Horizon #Initial singularity #Mathematical analysis #Physical cosmology #Physics #Quantum mechanics #Singularity #Theoretical physics #Ultimate fate of the universe #Universe #astro-ph
paper · pdf · doi:10.1016/s0375-9601(98)00617-3
published as Phys.Lett. A249 (1998) 37-45 · 18 LaTeX pages and 2 figures, accepted for publication in Physics Letters A
arxiv created 1998/09/10 · openalex publication_date 1998/11/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
One of the main drawbacks of standard cosmology, known as the horizon problem, was until now thought to be only solvable in an inflationary scenario. A delayed Big-Bang in an inhomogeneous universe is shown to solve this problem while leaving unimpaired the main successful features of the standard model.