Cosmological inflation models in the kinetic approximation
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Publication:2404885
DOI10.1134/S0040577917050166zbMath1371.83196OpenAlexW2621017811MaRDI QIDQ2404885
Publication date: 21 September 2017
Published in: Theoretical and Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0040577917050166
Cites Work
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- Total energy potential as a superpotential in integrable cosmological models
- Inflationary cosmological models without restrictions on a scalar field potential
- Exact cosmology and specification of an inflationary scenario
- On calculation of the cosmological parameters in exact models of inflation
- 20+ years of inflation
- Quantum cosmology with a complex \(\phi^4\) field at finite temperature
- A new type of isotropic cosmological models without singularity
- ON THE DYNAMICS OF A QUADRATIC SCALAR FIELD POTENTIAL
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Inflationary universe: A possible solution to the horizon and flatness problems
- Cosmological Imprint of an Energy Component with General Equation of State
- \(k\)-inflation
- An alternative to quintessence
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