TY  - JOUR
AU  - Easther, R.
AU  - Price, L. C.
AU  - Rasero, J.
PY  - 2014
DA  - 2014//
TI  - Inflating an inhomogeneous universe
T2  - J. Cosmol. Astropart. Phys.
JO  - Journal of Cosmology and Astroparticle Physics
SP  - 041
EP  - 16pp
VL  - 08
IS  - 8
PB  - Iop Publishing Ltd
KW  - inflation
KW  - initial conditions and eternal universe
KW  - physics of the early universe
AB  - While cosmological inflation can erase primordial inhomogeneities, it is possible that inflation may not begin in a significantly inhomogeneous universe. This issue is particularly pressing in multifield scenarios, where even the homogeneous dynamics may depend sensitively on the initial configuration. This paper presents an initial survey of the onset of inflation in multifield models, via qualitative lattice-based simulations that do not include local gravitational backreaction. Using hybrid inflation as a test model, our results suggest that small subhorizon inhomogeneities do play a key role in determining whether inflation begins in multifield scenarios. Interestingly, some configurations which do not inflate in the homogeneous limit "succeed" after inhomogeneity is included, while other initial configurations which inflate in the homogeneous limit "fail" when inhomogeneity is added.
SN  - 1475-7516
UR  - http://arxiv.org/abs/arXiv:1406.2869
UR  - https://doi.org/10.1088/1475-7516/2014/08/041
DO  - 10.1088/1475-7516/2014/08/041
LA  - English
N1  - WOS:000341848800041
ID  - Easther_etal2014
ER  -