Space-time slicing in Horndeski theories and its implications for non-singular bouncing solutions
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Publication:5022069
DOI10.1088/1475-7516/2018/02/007OpenAlexW2766538289MaRDI QIDQ5022069
Publication date: 18 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1710.05990
cosmological perturbation theoryphysics of the early universealternatives to inflationcosmic singularity
Related Items (10)
Cuscuton gravity as a classically stable limiting curvature theory ⋮ Subluminal cosmological bounce beyond Horndeski ⋮ DHOST bounce ⋮ Cyclic completion of the anamorphic universe ⋮ On efforts to decouple early universe cosmology and quantum gravity phenomenology ⋮ Evading the theoretical no-go theorem for nonsingular bounces in Horndeski/Galileon cosmology ⋮ Bouncing cosmology made simple ⋮ Unbraiding the bounce: superluminality around the corner ⋮ Bounce beyond Horndeski with GR asymptotics and γ-crossing ⋮ Sourcing curvature modes with entropy perturbations in non-singular bouncing cosmologies
Cites Work
- Inflation from Minkowski space
- Can Galileons support Lorentzian wormholes?
- Starting the universe: stable violation of the null energy condition and non-standard cosmologies
- The effective field theory of nonsingular cosmology
- Fully stable cosmological solutions with a non-singular classical bounce
- Effective field theory of cosmological perturbations
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- Gauge stability of 3 + 1 formulations of general relativity
- Numerical relativity using a generalized harmonic decomposition
- Cosmological bounce and Genesis beyond Horndeski
- Full bispectra from primordial scalar and tensor perturbations in the most general single-field inflation model
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