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A new model of dark matter distribution in galaxies
In the absence of the physical understanding of the phenomenon, different empirical laws have been used as approximation for distribution of dark matter in galaxies and clusters of galaxies. We suggest a new profile which is not empirical in nature, but motivated with the physical idea that what we...
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| Lenguaje: | eng |
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2013
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| Acceso en línea: | https://dx.doi.org/10.1007/s10509-013-1621-0 http://cds.cern.ch/record/1600908 |