Brane inflation driven by an arctan potential: CMB constraints and reheating
DOI10.1088/1475-7516/2022/07/024zbMath1506.83061arXiv2011.05264OpenAlexW4285402090MaRDI QIDQ5099369
S. Santos da Costa, F. A. Brito, R. M. P. Neves, Jailson S. Alcaniz
Publication date: 31 August 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2011.05264
Point estimation (62F10) Sampling theory, sample surveys (62D05) Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Supergravity (83E50) Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Constrained dynamics, Dirac's theory of constraints (70H45)
Related Items (1)
Cites Work
- Unnamed Item
- Unnamed Item
- First-order framework and domain-wall/brane-cosmology correspondence
- A domain wall description of brane inflation and observational aspects
- SUPERGRAVITY DESCRIPTION OF FIELD THEORIES ON CURVED MANIFOLDS AND A NO GO THEOREM
- DOMAIN WALL WORLD(S)
- de Sitter vacua in string theory
- String gas cosmology after Planck
- A Study of Accelerating Cosmologies from Superstring/M Theories
- Brane inflation.
This page was built for publication: Brane inflation driven by an arctan potential: CMB constraints and reheating