Quintessential α-attractor inflation: forecasts for Stage IV galaxy surveys
DOI10.1088/1475-7516/2021/04/006zbMath1485.83029arXiv2010.15822OpenAlexW3096284095MaRDI QIDQ5026089
Yashar Akrami, Santiago Casas, Valeri Vardanyan, Senwen Deng
Publication date: 7 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2010.15822
Diffraction, scattering (78A45) Geometrodynamics and the holographic principle (83E05) Quantum optics (81V80) Electromagnetic fields in general relativity and gravitational theory (83C50) Constrained dynamics, Dirac's theory of constraints (70H45) Dark matter and dark energy (83C56)
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- Superconformal inflationary \(\alpha\)-attractors
- Maximal supersymmetry and B-mode targets
- \( \overline{D3} \) induced geometric inflation
- Multi-field dark energy: cosmic acceleration on a steep potential
- Dark energy without fine tuning
- Warm quintessential inflation
- Evading Lyth bound in models of quintessential inflation
- \(\alpha\)-attractors: Planck, LHC and dark energy
- Quintessence: a review
- Reheating after quintessential inflation and gravitational waves
- The effect of Limber and flat-sky approximations on galaxy weak lensing
- Bayesian evidence for α-attractor dark energy models
- The string swampland constraints require multi-field inflation
- Reheating in quintessential inflation via gravitational production of heavy massive particles: a detailed analysis
- Inflation, braneworlds and quintessence
- The Landscape, the Swampland and the Era of Precision Cosmology
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