Smoothing and flattening the universe through slow contraction versus inflation
Journal Article
·
· Journal of Cosmology and Astroparticle Physics
- New York University, NY (United States)
- Princeton University, NJ (United States); Harvard University, Cambridge MA (United States)
- Oakland University, Rochester, MI (United States)
- Friedrich-Schiller-Universität Jena (Germany)
In a systematic study, we use an equivalent pair of improved numerical relativity codes based on a tetrad-formulation of the classical Einstein-scalar field equations to examine whether slow contraction or inflation (or both) can resolve the homogeneity, isotropy and flatness problems. Our finding, based on a set of gauge/frame invariant diagnostics and the models considered, is that slow contraction robustly and rapidly smooths and flattens spacetime beginning from initial conditions that are outside the perturbative regime of the flat Friedmann-Robertson-Walker metric, whereas inflation fails these tests. We present new numerical evidence supporting the conjecture that the combination of ultralocal evolution and an effective equation-of-state with pressure much greater than energy density is the key to having robust and rapid smoothing. The opposite of ultralocality occurs in expanding spacetimes, which is the leading obstruction to smoothing following a big bang.
- Research Organization:
- Princeton University, NJ (United States)
- Sponsoring Organization:
- National Science Foundation (NSF); Simons Foundation; USDOE Office of Science (SC), High Energy Physics (HEP)
- Grant/Contract Number:
- FG02-91ER40671; SC0007968
- OSTI ID:
- 2484172
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 07 Vol. 2024; ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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