WARM-LOGAMEDIATE INFLATIONARY UNIVERSE MODEL

2012/04/09 by Ramón Herrera, Ramon Herrera, Marco Olivares · 1 citation
Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Context (archaeology) #Cosmology #Cosmology and Gravitation Theories #Dark energy #Dissipative system #Galaxies: Formation, Evolution, Phenomena #History #Inflation (cosmology) #Inflationary epoch #Metric expansion of space #Physics #Quantum mechanics #Theoretical physics #Universe #gr-qc

paper · pdf · doi:10.1142/s0218271812500472

16 pages, 2 figures. Accepted for publication in IJMPD. arXiv admin note: text overlap with arXiv:1108.1371

openalex publication_date 2012/04/09 · arxiv created 2012/05/10 · arxiv updated 2015/06/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Warm inflationary universe models in the context of logamediate expansion are studied. General conditions required for these models to be realizable and discussed. This study is done in the weak and strong dissipative regimes. The parameters of our models are constrained from the observational data.

Citations

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Cited by

• Inflationary weak anisotropic model with general dissipation coefficient