The boundary proposal.
Saved in:
| Title: | The boundary proposal. |
|---|---|
| Authors: | Friedrich, Bjoern1 (AUTHOR) friedrich@thphys.uni-heidelberg.de, Hebecker, Arthur1 (AUTHOR) a.hebecker@thphys.uni-heidelberg.de |
| Source: | Physics Letters B. Sep2024, Vol. 856, pN.PAG-N.PAG. 1p. |
| Subjects: | Branes, Torus, Spacetime, Spheres, Universe |
| Abstract: | 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 Proposal, one may then be able to create a compact, flat torus universe from nothing, without any exponential suppression or enhancement factors. [ABSTRACT FROM AUTHOR] |
| Copyright of Physics Letters B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
| FullText | Text: Availability: 0 |
|---|---|
| Header | DbId: egs DbLabel: Engineering Source An: 179274052 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
| IllustrationInfo | |
| Items | – Name: Title Label: Title Group: Ti Data: The boundary proposal. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Friedrich%2C+Bjoern%22">Friedrich, Bjoern</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> friedrich@thphys.uni-heidelberg.de</i><br /><searchLink fieldCode="AR" term="%22Hebecker%2C+Arthur%22">Hebecker, Arthur</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> a.hebecker@thphys.uni-heidelberg.de</i> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Physics+Letters+B%22">Physics Letters B</searchLink>. Sep2024, Vol. 856, pN.PAG-N.PAG. 1p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Branes%22">Branes</searchLink><br /><searchLink fieldCode="DE" term="%22Torus%22">Torus</searchLink><br /><searchLink fieldCode="DE" term="%22Spacetime%22">Spacetime</searchLink><br /><searchLink fieldCode="DE" term="%22Spheres%22">Spheres</searchLink><br /><searchLink fieldCode="DE" term="%22Universe%22">Universe</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: 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 Proposal, one may then be able to create a compact, flat torus universe from nothing, without any exponential suppression or enhancement factors. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Physics Letters B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=179274052 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1016/j.physletb.2024.138946 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 1 StartPage: N.PAG Subjects: – SubjectFull: Branes Type: general – SubjectFull: Torus Type: general – SubjectFull: Spacetime Type: general – SubjectFull: Spheres Type: general – SubjectFull: Universe Type: general Titles: – TitleFull: The boundary proposal. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Friedrich, Bjoern – PersonEntity: Name: NameFull: Hebecker, Arthur IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 09 Text: Sep2024 Type: published Y: 2024 Identifiers: – Type: issn-print Value: 03702693 Numbering: – Type: volume Value: 856 Titles: – TitleFull: Physics Letters B Type: main |
| ResultId | 1 |