SPATIALLY FLAT FRW MODELS WITH A NONMINIMALLY COUPLED GHOST SCALAR FIELD AND PERFECT FLUID IN EINSTEIN–CARTAN THEORY
DOI10.1142/S0218271812500010zbMath1263.83128OpenAlexW2042090610WikidataQ125824354 ScholiaQ125824354MaRDI QIDQ4914222
Publication date: 18 April 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0218271812500010
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (5)
Cites Work
- Bianchi-I cosmologies with a scalar field and an ultrarelativistic gas in Einstein-Cartan theory
- Propagating torsion from first principles
- Dark Energy
- Cosmology with polynomial potentials of the fourth degree in Einstein–Cartan theory
- Regular Phantom Black Holes
- RECONSTRUCTING DARK ENERGY
- Exact isotropic scalar field cosmologies in Einstein–Cartan theory
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- General relativity with spin and torsion: Foundations and prospects
- GHOST COSMOLOGY: EXACT SOLUTIONS, TRANSITIONS BETWEEN STANDARD COSMOLOGIES AND GHOST EVOLUTION
- Analysis of inflationary cosmological models in gauge theories of gravitation
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