A differential representation of cosmological wavefunctions
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Publication:2092533
DOI10.1007/JHEP04(2022)012MaRDI QIDQ2092533
Publication date: 2 November 2022
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2112.01619
models of quantum gravityspace-time symmetrieseffective field theoriesearly universe particle physics
Related Items (17)
From amplitudes to contact cosmological correlators ⋮ Cutting cosmological correlators ⋮ Soft theorems for boosts and other time symmetries ⋮ Effective field theories and cosmological scattering equations ⋮ Soft limits of the wavefunction in exceptional scalar theories ⋮ The cosmological tree theorem ⋮ Boostless cosmological collider bootstrap ⋮ The analytic wavefunction ⋮ The graviton four-point function in de Sitter space ⋮ Bootstrapping multi-field inflation: non-Gaussianities from light scalars revisited ⋮ Leading loops in cosmological correlators ⋮ Nonanalyticity and on-shell factorization of inflation correlators at all loop orders ⋮ Cosmological bootstrap in slow motion ⋮ On the differential representation and color-kinematics duality of AdS boundary correlators ⋮ On-shell correlators and color-kinematics duality in curved symmetric spacetimes ⋮ Bootstrapping large graviton non-Gaussianities ⋮ Cosmological scattering equations at tree-level and one-loop
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