The Boundary Proposal ...
One of the leading ideas for the beginning of the Universe is the Hartle-Hawking `No-Boundary Proposal.' Since the Cobordism Conjecture claims that any spacetime allows for a dynamical boundary, we suggest that one may equally well consider a `Boundary Proposal'. Specifically, the correspo...
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Online Access: | https://dx.doi.org/10.48550/arxiv.2403.18892 https://arxiv.org/abs/2403.18892 |
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ftdatacite:10.48550/arxiv.2403.18892 2024-04-28T08:38:49+00:00 The Boundary Proposal ... Friedrich, Bjoern Hebecker, Arthur 2024 https://dx.doi.org/10.48550/arxiv.2403.18892 https://arxiv.org/abs/2403.18892 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Physics - Theory hep-th General Relativity and Quantum Cosmology gr-qc FOS Physical sciences article Article Preprint CreativeWork 2024 ftdatacite https://doi.org/10.48550/arxiv.2403.18892 2024-04-02T12:56:11Z One of the leading ideas for the beginning of the Universe is the Hartle-Hawking `No-Boundary Proposal.' Since the Cobordism Conjecture claims that any spacetime allows for a dynamical boundary, we suggest that one may equally well consider a `Boundary Proposal'. Specifically, the corresponding euclidean instanton is a sphere with two holes around north and south pole cut out. Analogously to the Hartle-Hawking proposal, the sphere is then cut in two at the equator and half of it is dropped. The equator is glued to an expanding Lorentzian de Sitter space, implementing a beginning of the Universe with a spacelike spherical boundary at its earliest moment. This process is in principle on equal footing with the one based on the no-boundary instanton. In fact, if the Linde-Vilenkin sign choice is used, this `Boundary' creation process may even dominate. An intriguing implication arises if tensionless end-of-the-world branes, as familiar from type-IIA or M-theory, are available: Analogously to the Boundary ... : 14 pages, 3 figures ... Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Physics - Theory hep-th General Relativity and Quantum Cosmology gr-qc FOS Physical sciences |
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High Energy Physics - Theory hep-th General Relativity and Quantum Cosmology gr-qc FOS Physical sciences Friedrich, Bjoern Hebecker, Arthur The Boundary Proposal ... |
topic_facet |
High Energy Physics - Theory hep-th General Relativity and Quantum Cosmology gr-qc FOS Physical sciences |
description |
One of the leading ideas for the beginning of the Universe is the Hartle-Hawking `No-Boundary Proposal.' Since the Cobordism Conjecture claims that any spacetime allows for a dynamical boundary, we suggest that one may equally well consider a `Boundary Proposal'. Specifically, the corresponding euclidean instanton is a sphere with two holes around north and south pole cut out. Analogously to the Hartle-Hawking proposal, the sphere is then cut in two at the equator and half of it is dropped. The equator is glued to an expanding Lorentzian de Sitter space, implementing a beginning of the Universe with a spacelike spherical boundary at its earliest moment. This process is in principle on equal footing with the one based on the no-boundary instanton. In fact, if the Linde-Vilenkin sign choice is used, this `Boundary' creation process may even dominate. An intriguing implication arises if tensionless end-of-the-world branes, as familiar from type-IIA or M-theory, are available: Analogously to the Boundary ... : 14 pages, 3 figures ... |
format |
Article in Journal/Newspaper |
author |
Friedrich, Bjoern Hebecker, Arthur |
author_facet |
Friedrich, Bjoern Hebecker, Arthur |
author_sort |
Friedrich, Bjoern |
title |
The Boundary Proposal ... |
title_short |
The Boundary Proposal ... |
title_full |
The Boundary Proposal ... |
title_fullStr |
The Boundary Proposal ... |
title_full_unstemmed |
The Boundary Proposal ... |
title_sort |
boundary proposal ... |
publisher |
arXiv |
publishDate |
2024 |
url |
https://dx.doi.org/10.48550/arxiv.2403.18892 https://arxiv.org/abs/2403.18892 |
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South pole |
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South pole |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.2403.18892 |
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