Autor: |
Taylor, Peter, Massey, Richard, Jauzac, Mathilde, Courbin, Frédéric, Harvey, David, Joseph, Rémy, Robertson, Andrew |
Rok vydání: |
2017 |
Předmět: |
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Druh dokumentu: |
Working Paper |
DOI: |
10.1093/mnras/stx855 |
Popis: |
Simulations of self-interacting dark matter (SIDM) predict that dark matter should lag behind galaxies during a collision. If the interaction is mediated by a high-mass force carrier, the distribution of dark matter can also develop asymmetric dark matter tails. To search for this asymmetry, we compute the gravitational lensing properties of a mass distribution with a free {\em skewness} parameter. We apply this to the dark matter around the four central galaxies in cluster Abell~3827. In the galaxy whose dark matter peak has previously been found to be offset, we tentatively measure a skewness $s=0.23^{+0.05}_{-0.22}$ in the same direction as the peak offset. Our method may be useful in future gravitational lensing analyses of colliding galaxy clusters and merging galaxies. |
Databáze: |
arXiv |
Externí odkaz: |
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