Details
Originalsprache | Englisch |
---|---|
Aufsatznummer | 030 |
Fachzeitschrift | Journal of Cosmology and Astroparticle Physics |
Jahrgang | 2020 |
Ausgabenummer | 8 |
Publikationsstatus | Veröffentlicht - 13 Aug. 2020 |
Abstract
We present numerical relativity simulations of cosmological scenarios in which the universe is smoothed and flattened by undergoing a phase of slow contraction and test their sensitivity to a wide range of initial conditions. Our numerical scheme enables the variation of all freely specifiable physical quantities that characterize the initial spatial hypersurface, such as the initial shear and spatial curvature contributions as well as the initial field and velocity distributions of the scalar that drives the cosmological evolution. In particular, we include initial conditions that are far outside the perturbative regime of the well-known attractor scaling solution. We complement our numerical results by analytically performing a complete dynamical systems analysis and show that the two approaches yield consistent results.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
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in: Journal of Cosmology and Astroparticle Physics, Jahrgang 2020, Nr. 8, 030, 13.08.2020.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Robustness of slow contraction to cosmic initial conditions
AU - Ijjas, Anna
AU - Cook, William G.
AU - Pretorius, Frans
AU - Steinhardt, Paul J.
AU - Davies, Elliot Y.
PY - 2020/8/13
Y1 - 2020/8/13
N2 - We present numerical relativity simulations of cosmological scenarios in which the universe is smoothed and flattened by undergoing a phase of slow contraction and test their sensitivity to a wide range of initial conditions. Our numerical scheme enables the variation of all freely specifiable physical quantities that characterize the initial spatial hypersurface, such as the initial shear and spatial curvature contributions as well as the initial field and velocity distributions of the scalar that drives the cosmological evolution. In particular, we include initial conditions that are far outside the perturbative regime of the well-known attractor scaling solution. We complement our numerical results by analytically performing a complete dynamical systems analysis and show that the two approaches yield consistent results.
AB - We present numerical relativity simulations of cosmological scenarios in which the universe is smoothed and flattened by undergoing a phase of slow contraction and test their sensitivity to a wide range of initial conditions. Our numerical scheme enables the variation of all freely specifiable physical quantities that characterize the initial spatial hypersurface, such as the initial shear and spatial curvature contributions as well as the initial field and velocity distributions of the scalar that drives the cosmological evolution. In particular, we include initial conditions that are far outside the perturbative regime of the well-known attractor scaling solution. We complement our numerical results by analytically performing a complete dynamical systems analysis and show that the two approaches yield consistent results.
KW - Alternatives to ination
KW - Cosmological simulations
KW - Gravity
KW - Physics of the early universe
UR - http://www.scopus.com/inward/record.url?scp=85090875033&partnerID=8YFLogxK
U2 - 10.48550/arXiv.2006.04999
DO - 10.48550/arXiv.2006.04999
M3 - Article
AN - SCOPUS:85090875033
VL - 2020
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
SN - 1475-7516
IS - 8
M1 - 030
ER -