Dynamics of logamediate and intermediate scenarios in the Dark energy filled universe
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Publication:2429965
DOI10.1007/s10773-010-0617-6zbMath1210.83047arXiv1012.1445OpenAlexW3102789487MaRDI QIDQ2429965
Ujjal Debnath, Piyali Bagchi Khatua
Publication date: 5 April 2011
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1012.1445
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)
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Cites Work
- Generation of electromagnetic fields in string cosmology with a massive scalar field on the anti-D-brane
- The gravitating perfect fluid-scalar field equations: quintessence and tachyonic matter
- DYNAMICS OF DARK ENERGY
- Role of modified Chaplygin gas in accelerated universe
- FIELD THEORY OF TACHYON MATTER
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- INFLATIONARY UNIVERSE WITH TACHYON FIELD
- An alternative to quintessence