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http://hdl.handle.net/2248/6526
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DC Field | Value | Language |
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dc.contributor.author | Sivaram, C | - |
dc.contributor.author | Arun, K | - |
dc.contributor.author | Kiren, O. V | - |
dc.date.accessioned | 2013-12-26T13:21:18Z | - |
dc.date.available | 2013-12-26T13:21:18Z | - |
dc.date.issued | 2013-11-29 | - |
dc.identifier.citation | The Open Astronomy Journal, Vol. 6, pp. 90-97 | en |
dc.identifier.issn | 1874-3811 | - |
dc.identifier.uri | http://hdl.handle.net/2248/6526 | - |
dc.description | This is an open access article licensed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/3.0/) which permits unrestricted, non-commercial use, distribution and reproduction in any medium, provided the work is properly cited. | en |
dc.description.abstract | In recent work, a new cosmological paradigm implied a mass-radius relation, suggesting a universal tension related to the background dark energy (cosmological constant), leading to an energy per unit area that holds for structures from atomic nuclei to clusters of galaxies. Here we explore some of the consequences that arise from such a universal tension. | en |
dc.language.iso | en | en |
dc.publisher | Bentham Open | en |
dc.relation.uri | http://dx.doi.org/10.2174/1874381101306010090 | en |
dc.rights | © Sivaram and Arun; Licensee Bentham Open | en |
dc.subject | Universal Tension | en |
dc.subject | Dark Energy | en |
dc.subject | Atomic Nuclei | en |
dc.subject | Galaxies | en |
dc.subject | Galaxy Clusters | en |
dc.title | Some Consequences of a Universal Tension Arising from Dark Energy for Structures from Atomic Nuclei to Galaxy Clusters | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Some Consequences of a Universal Tension Arising.pdf | 700.74 kB | Adobe PDF | View/Open |
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