Inflation, Dark Matter, and Dark Energy in the String Landscape

DOI10.1103/PhysRevLett.97.161301zbMath1228.83137arXivastro-ph/0605205OpenAlexW1992788985WikidataQ59450589 ScholiaQ59450589MaRDI QIDQ3107843

Andrew R. Liddle, L. Arturo Ureña - López

Publication date: 26 December 2011

Published in: Physical Review Letters (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0605205

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30)

Related Items

SCALAR POTENTIALS OUT OF CANONICAL QUANTUM COSMOLOGY ⋮ Non-minimal coupling inflation and dark matter under the ℤ₃ symmetry ⋮ The universe dynamics from topological considerations ⋮ Fractional action cosmology with variable order parameter ⋮ Inflation and dark matter in the inert doublet model ⋮ A new unified dark fluid model and its cosmic constraint ⋮ Effective cosmological constant within the expanding axion universe ⋮ \(f(R)\) theories ⋮ INFLATION AS A RESPONSE TO PROTECT THE HOLOGRAPHIC PRINCIPLE ⋮ Analysis of scalar field cosmology with phase space deformations ⋮ Hidden inflaton dark matter ⋮ Unifying dark matter, dark energy and inflation with a fuzzy dark fluid ⋮ Supersymmetric ν-inflaton Dark Matter ⋮ Emerging the dark sector from thermodynamics of cosmological systems with constant pressure

Cites Work

• ON THE NATURE OF DARK MATTER
• Quantization of four-form fluxes and dynamical neutralization of the cosmological constant
• Generating the curvature perturbation without an inflaton