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

zbMATH Keywords

inflationmodified gravitystatistical sampling techniquescosmological parameters from CMBR

Mathematics Subject Classification ID

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)

String cosmology: from the early universe to today

Cites Work

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• 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.

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