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Energy conditions allow eternal inflation
Eternal inflation requires upward fluctuations of the energy in a Hubble volume, which appear to violate the energy conditions. In particular, a scalar field in an inflating spacetime should obey the averaged null energy condition, which seems to rule out eternal inflation. Here we show how eternal...
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Published in: | Journal of cosmology and astroparticle physics 2021-03, Vol.2021 (3), p.97 |
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container_issue | 3 |
container_start_page | 97 |
container_title | Journal of cosmology and astroparticle physics |
container_volume | 2021 |
creator | Kontou, Eleni-Alexandra Olum, Ken D. |
description | Eternal inflation requires upward fluctuations of the energy in a
Hubble volume, which appear to violate the energy conditions. In
particular, a scalar field in an inflating spacetime should obey the
averaged null energy condition, which seems to rule out eternal
inflation. Here we show how eternal inflation is possible when energy
conditions (even the null energy condition) are obeyed. The critical
point is that energy conditions restrict the evolution of any single
quantum state, while the process of eternal inflation involves
repeatedly selecting a subsector of the previous state, so there is no
single state where the conditions are violated. |
doi_str_mv | 10.1088/1475-7516/2021/03/097 |
format | article |
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Hubble volume, which appear to violate the energy conditions. In
particular, a scalar field in an inflating spacetime should obey the
averaged null energy condition, which seems to rule out eternal
inflation. Here we show how eternal inflation is possible when energy
conditions (even the null energy condition) are obeyed. The critical
point is that energy conditions restrict the evolution of any single
quantum state, while the process of eternal inflation involves
repeatedly selecting a subsector of the previous state, so there is no
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Hubble volume, which appear to violate the energy conditions. In
particular, a scalar field in an inflating spacetime should obey the
averaged null energy condition, which seems to rule out eternal
inflation. Here we show how eternal inflation is possible when energy
conditions (even the null energy condition) are obeyed. The critical
point is that energy conditions restrict the evolution of any single
quantum state, while the process of eternal inflation involves
repeatedly selecting a subsector of the previous state, so there is no
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Hubble volume, which appear to violate the energy conditions. In
particular, a scalar field in an inflating spacetime should obey the
averaged null energy condition, which seems to rule out eternal
inflation. Here we show how eternal inflation is possible when energy
conditions (even the null energy condition) are obeyed. The critical
point is that energy conditions restrict the evolution of any single
quantum state, while the process of eternal inflation involves
repeatedly selecting a subsector of the previous state, so there is no
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ispartof | Journal of cosmology and astroparticle physics, 2021-03, Vol.2021 (3), p.97 |
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language | eng |
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source | Institute of Physics:Jisc Collections:IOP Publishing Read and Publish 2024-2025 (Reading List) |
subjects | Critical point Energy Inflation (cosmology) Scalars |
title | Energy conditions allow eternal inflation |
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