Cosmology with non-linear scalar field

DOI10.1007/s10509-010-0292-3zbMath1187.85033OpenAlexW2005804412MaRDI QIDQ973725

Wei Fang, H. Q. Lu, Z. G. Huang, Kai Zhang

Publication date: 26 May 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0292-3

zbMATH Keywords

quintessencedark energysquare potentialnon-linear scalar field

Mathematics Subject Classification ID

Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Cites Work

• The consistent result of cosmological constant from quantum cosmology and inflation with Born-Infeld scalar field
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• A COMPARISON OF QUINTESSENCE AND NON-LINEAR BORN–INFELD SCALAR FIELD USING GOLD SUPERNOVA DATA
• Constraints on the cosmic equation of state: Age conflict versus phantom energy
• PHANTOM COSMOLOGY WITH A NONLINEAR BORN–INFELD TYPE SCALAR FIELD
• OBSERVATIONAL CONSTRAINTS ON DARK ENERGY MODEL
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• Cosmologies with a general non-canonical scalar field
• An alternative to quintessence

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