2013/05/08 by Nilanjana Mahata, Subenoy Chakraborty, Mahata, Nilanjana +1
Physics and Astronomy · #Astro and Planetary Science #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Stellar, planetary, and galactic studies #gr-qc
paper · pdf · doi:10.48550/arxiv.1305.1702
8 pages, 4 figures
arxiv created 2013/05/08 · openalex publication_date 2013/05/08 · arxiv updated 2013/05/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The work deals with homogeneous and isotropic, flat FRW model of the universe which is filled up with non-interacting dark matter and dark energy to compatible with recent observational evidences. By choosing the dark energy in the form of a dilatonic scalar field, the evolution equations are reduced to an autonomous system. A phase space analysis is done around the critical points and stability criteria is examined. Finally, cosmological implications of the nature of the critical points are discussed.