Warm-viscous inflation model on the brane in light of Planck data
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Publication:3466373
DOI10.1088/0264-9381/32/23/235005zbMath1329.83216arXiv1312.2832OpenAlexW2272036747MaRDI QIDQ3466373
Mohammad R. Setare, Vahid Kamali
Publication date: 1 February 2016
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1312.2832
Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Stability and instability of geophysical and astrophysical flows (76E20) Astrophysical cosmology (85A40)
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Cites Work
- Cosmological perturbations in warm-tachyon inflationary universe model with viscous pressure on the brane
- The hierarchy problem and new dimensions at a millimeter
- The importance of being warm (during inflation)
- Heterotic and type I string dynamics from eleven dimensions
- Warm-intermediate inflationary universe model with viscous pressure in high dissipative regime
- Dissipative effects in the effective field theory of inflation
- Cosmological solutions of Hořava-Witten theory
- WARM INFLATION MODEL BUILDING
- Nonequilibrium Quantum Field Theory
- Cosmological Inflation and Large-Scale Structure
- Dirichlet Branes and Ramond-Ramond Charges
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- WARM TACHYONIC INFLATION IN A WARPED BACKGROUND
- Inflationary universe: A possible solution to the horizon and flatness problems
- Cosmological perturbations from multi-field inflation in generalized Einstein theories
- Density perturbations in warm inflation and COBE normalization