A (semi)-exact Hamiltonian for the curvature perturbation ζ
From MaRDI portal
Publication:5090130
DOI10.1088/1361-6382/AC7768zbMath1498.83055arXiv2206.04819OpenAlexW4281935703WikidataQ114096927 ScholiaQ114096927MaRDI QIDQ5090130
Publication date: 15 July 2022
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2206.04819
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Perturbations in context of PDEs (35B20) Constrained dynamics, Dirac's theory of constraints (70H45)
Cites Work
- Holography for inflation using conformal perturbation theory
- On loops in inflation
- The cosmological bootstrap: inflationary correlators from symmetries and singularities
- Stochastic quantum gravitational inflation
- A concise introduction to perturbation theory in cosmology
- The Cosmological Optical Theorem
- Initial wave function of the universe is arbitrary
This page was built for publication: A (semi)-exact Hamiltonian for the curvature perturbation ζ