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• W3100101589 abstract "A non-topological soliton model with a repulsive scalar self-interaction of the Emden type provides a constant-density core, similarly as the empirical Burkert profile of dark matter (DM) haloes. As a further test, we derive the gravitational lens properties of our model, in particular, the demarcation curves between ‘weak’ and ‘strong’ lensing. Accordingly, strong lensing with typically three images is almost three times more probable for our solitonic model than for the Burkert fit. Moreover, some prospective consequences of a possible flattening of DM haloes are indicated." @default.
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• W3100101589 date "2006-05-08" @default.
• W3100101589 modified "2023-10-01" @default.
• W3100101589 title "Scalar field haloes as gravitational lenses" @default.
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• W3100101589 doi "https://doi.org/10.1111/j.1365-2966.2006.10330.x" @default.
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