Details
Originalsprache | Englisch |
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Aufsatznummer | 013 |
Fachzeitschrift | Journal of Cosmology and Astroparticle Physics |
Jahrgang | 2021 |
Ausgabenummer | 6 |
Publikationsstatus | Veröffentlicht - 8 Juni 2021 |
Abstract
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
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in: Journal of Cosmology and Astroparticle Physics, Jahrgang 2021, Nr. 6, 013, 08.06.2021.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Ultralocality and slow contraction
AU - Ijjas, Anna
AU - Sullivan, Andrew P.
AU - Pretorius, Frans
AU - Steinhardt, Paul J.
AU - Cook, William G.
PY - 2021/6/8
Y1 - 2021/6/8
N2 - We study the detailed process by which slow contraction smooths and flattens the universe using an improved numerical relativity code that accepts initial conditions with non-perturbative deviations from homogeneity and isotropy along two independent spatial directions. Contrary to common descriptions of the early universe, we find that the geometry first rapidly converges to an inhomogeneous, spatially-curved and anisotropic ultralocal state in which all spatial gradient contributions to the equations of motion decrease as an exponential in time to negligible values. This is followed by a second stage in which the geometry converges to a homogeneous, spatially flat and isotropic spacetime. In particular, the decay appears to follow the same history whether the entire spacetime or only parts of it are smoothed by the end of slow contraction.
AB - We study the detailed process by which slow contraction smooths and flattens the universe using an improved numerical relativity code that accepts initial conditions with non-perturbative deviations from homogeneity and isotropy along two independent spatial directions. Contrary to common descriptions of the early universe, we find that the geometry first rapidly converges to an inhomogeneous, spatially-curved and anisotropic ultralocal state in which all spatial gradient contributions to the equations of motion decrease as an exponential in time to negligible values. This is followed by a second stage in which the geometry converges to a homogeneous, spatially flat and isotropic spacetime. In particular, the decay appears to follow the same history whether the entire spacetime or only parts of it are smoothed by the end of slow contraction.
KW - alternatives to inflation
KW - cosmological simulations
KW - gravity
KW - physics of the early universe
UR - http://www.scopus.com/inward/record.url?scp=85108434262&partnerID=8YFLogxK
U2 - 10.48550/arXiv.2103.00584
DO - 10.48550/arXiv.2103.00584
M3 - Article
VL - 2021
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
SN - 1475-7516
IS - 6
M1 - 013
ER -