Using atom interferometry to detect dark energy.
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| Title: | Using atom interferometry to detect dark energy. |
|---|---|
| Authors: | Burrage, Clare1, Copeland, Edmund J.1 |
| Source: | Contemporary Physics. Jun2016, Vol. 57 Issue 2, p164-176. 13p. |
| Subjects: | Dark energy, Interferometry, Metaphysical cosmology, Parsec, Atom interferometers |
| Abstract: | We review the tantalising prospect that the first evidence for the dark energy driving the observed acceleration of the universe on giga-parsec scales may be found through metre scale laboratory-based atom interferometry experiments. To do that, we first introduce the idea that scalar fields could be responsible for dark energy and show that in order to be compatible with fifth force constraints, these fields must have a screening mechanism which hides their effects from us within the solar system. Particular emphasis is placed on one such screening mechanism known as the chameleon effect where the field’s mass becomes dependent on the environment. The way the field behaves in the presence of a spherical source is determined and we then go on to show how in the presence of the kind of high vacuum associated with atom interferometry experiments, and when the test particle is an atom, it is possible to use the associated interference pattern to place constraints on the acceleration due to the fifth force of the chameleon field – this has already been used to rule out large regions of the chameleon parameter space and maybe one day will be able to detect the force due to the dark energy field in the laboratory. [ABSTRACT FROM AUTHOR] |
| Copyright of Contemporary Physics is the property of Taylor & Francis Ltd 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 |
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| Header | DbId: egs DbLabel: Engineering Source An: 114607275 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Using atom interferometry to detect dark energy. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Burrage%2C+Clare%22">Burrage, Clare</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Copeland%2C+Edmund+J%2E%22">Copeland, Edmund J.</searchLink><relatesTo>1</relatesTo> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Contemporary+Physics%22">Contemporary Physics</searchLink>. Jun2016, Vol. 57 Issue 2, p164-176. 13p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Dark+energy%22">Dark energy</searchLink><br /><searchLink fieldCode="DE" term="%22Interferometry%22">Interferometry</searchLink><br /><searchLink fieldCode="DE" term="%22Metaphysical+cosmology%22">Metaphysical cosmology</searchLink><br /><searchLink fieldCode="DE" term="%22Parsec%22">Parsec</searchLink><br /><searchLink fieldCode="DE" term="%22Atom+interferometers%22">Atom interferometers</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: We review the tantalising prospect that the first evidence for the dark energy driving the observed acceleration of the universe on giga-parsec scales may be found through metre scale laboratory-based atom interferometry experiments. To do that, we first introduce the idea that scalar fields could be responsible for dark energy and show that in order to be compatible with fifth force constraints, these fields must have a screening mechanism which hides their effects from us within the solar system. Particular emphasis is placed on one such screening mechanism known as the chameleon effect where the field’s mass becomes dependent on the environment. The way the field behaves in the presence of a spherical source is determined and we then go on to show how in the presence of the kind of high vacuum associated with atom interferometry experiments, and when the test particle is an atom, it is possible to use the associated interference pattern to place constraints on the acceleration due to the fifth force of the chameleon field – this has already been used to rule out large regions of the chameleon parameter space and maybe one day will be able to detect the force due to the dark energy field in the laboratory. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Contemporary Physics is the property of Taylor & Francis Ltd 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.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1080/00107514.2015.1060058 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 13 StartPage: 164 Subjects: – SubjectFull: Dark energy Type: general – SubjectFull: Interferometry Type: general – SubjectFull: Metaphysical cosmology Type: general – SubjectFull: Parsec Type: general – SubjectFull: Atom interferometers Type: general Titles: – TitleFull: Using atom interferometry to detect dark energy. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Burrage, Clare – PersonEntity: Name: NameFull: Copeland, Edmund J. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 06 Text: Jun2016 Type: published Y: 2016 Identifiers: – Type: issn-print Value: 00107514 Numbering: – Type: volume Value: 57 – Type: issue Value: 2 Titles: – TitleFull: Contemporary Physics Type: main |
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