Bouncing cosmology made simple
DOI10.1088/1361-6382/aac482zbMath1409.83236arXiv1803.01961OpenAlexW3106365199WikidataQ129841873 ScholiaQ129841873MaRDI QIDQ3120804
Anna Ijjas, Paul J. Steinhardt
Publication date: 19 March 2019
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1803.01961
flatness problemsingularity problembouncing cosmologytensor-to-scalar ratiohomogeneity problemekyprotic universe
Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Space-time singularities, cosmic censorship, etc. (83C75) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25)
Related Items (22)
Cites Work
- The effective field theory of nonsingular cosmology
- Fully stable cosmological solutions with a non-singular classical bounce
- Bouncing cosmologies: progress and problems
- Why the Cosmological Constant Is Small and Positive
- Cosmological bounce and Genesis beyond Horndeski
- Space-time slicing in Horndeski theories and its implications for non-singular bouncing solutions
- Inflationary universe: A possible solution to the horizon and flatness problems
- Note on the production of scale-invariant entropy perturbation in the Ekpyrotic universe
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