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Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings
An exact solution of Einstein's field equations for a point mass surrounded by a static, spherically symmetric fluid of strings is presented. The solution is singular at the origin. Near the string cloud limit there is a $1/r$ correction to Newton's force law. It is noted that at large dis...
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Lenguaje: | eng |
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1994
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Acceso en línea: | https://dx.doi.org/10.1007/BF02107935 http://cds.cern.ch/record/274211 |
_version_ | 1780887375115714560 |
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author | Soleng, Harald H. |
author_facet | Soleng, Harald H. |
author_sort | Soleng, Harald H. |
collection | CERN |
description | An exact solution of Einstein's field equations for a point mass surrounded by a static, spherically symmetric fluid of strings is presented. The solution is singular at the origin. Near the string cloud limit there is a $1/r$ correction to Newton's force law. It is noted that at large distances and small accelerations, this law coincides with the phenomenological force law invented by Milgrom in order to explain the flat rotation curves of galaxies without introducing dark matter. When interpreted in the context of a cosmological model with a string fluid, the new solution naturally explains why the critical acceleration of Milgrom is of the same order of magnitude as the Hubble parameter. |
id | cern-274211 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1994 |
record_format | invenio |
spelling | cern-2742112019-09-30T06:29:59Zdoi:10.1007/BF02107935http://cds.cern.ch/record/274211engSoleng, Harald H.Dark matter and non-newtonian gravity from general relativity coupled to a fluid of stringsGeneral Relativity and CosmologyAn exact solution of Einstein's field equations for a point mass surrounded by a static, spherically symmetric fluid of strings is presented. The solution is singular at the origin. Near the string cloud limit there is a $1/r$ correction to Newton's force law. It is noted that at large distances and small accelerations, this law coincides with the phenomenological force law invented by Milgrom in order to explain the flat rotation curves of galaxies without introducing dark matter. When interpreted in the context of a cosmological model with a string fluid, the new solution naturally explains why the critical acceleration of Milgrom is of the same order of magnitude as the Hubble parameter.gr-qc/9412053NORDITA-94-69NORDITA-94-73-Poai:cds.cern.ch:2742111994-12-20 |
spellingShingle | General Relativity and Cosmology Soleng, Harald H. Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title | Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title_full | Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title_fullStr | Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title_full_unstemmed | Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title_short | Dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
title_sort | dark matter and non-newtonian gravity from general relativity coupled to a fluid of strings |
topic | General Relativity and Cosmology |
url | https://dx.doi.org/10.1007/BF02107935 http://cds.cern.ch/record/274211 |
work_keys_str_mv | AT solengharaldh darkmatterandnonnewtoniangravityfromgeneralrelativitycoupledtoafluidofstrings |