INFLATION AS AN ATTRACTOR IN SCALAR COSMOLOGY
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Publication:2866974
DOI10.1142/S0217732313500892zbMath1277.83112arXiv1211.0604OpenAlexW2161331995MaRDI QIDQ2866974
Publication date: 10 December 2013
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1211.0604
Related Items (2)
Quadratic integrals of a multi-scalar cosmological model ⋮ Multiscalar field models: Interaction potentials, wave functions and cosmological solutions
Cites Work
- Exact solution of scalar field cosmology with exponential potentials and transient acceleration
- First-order formalism and dark energy
- Construction of exact solutions in two-field cosmological models
- Stable exact solutions in cosmological models with two scalar fields
- A phase transition between small- and large-field models of inflation
- Cosmic no-hair theorem in homogeneous spacetimes. I. Bianchi models
- Isotropic and anisotropic N -dimensional cosmologies with exponential potentials
- General solution to two-scalar field cosmologies with exponential potentials
- Cosmology with exponential potentials
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