Misc,

Constraints on dark matter annihilation in $ømega$ Centauri

, , , , , , , , and .
(2020)cite arxiv:2005.11962Comment: 7 pages, 4 figures, 1 table.

Abstract

We present an analysis of Murchison Widefield Array radio telescope data from $ømega$ Cen, possibly a stripped dwarf spheroidal galaxy core captured by our Galaxy. Recent interpretations of Fermi-LAT $\gamma$-ray data by Brown et al. (2019) and Reynoso-Cordova et al. (2019) suggest that $ømega$ Cen may contain significant Dark Matter. We utilise their best-fit Dark Matter annihilation models, and an estimate of the magnetic field strength in $ømega$ Cen, to calculate the expected radio synchrotron signal from annihilation, and show that one can usefully rule out significant parts of the magnetic field - diffusion coefficient plane using the current observational limits. Improvement by a factor of 10-100 on these limits could constrain the models even more tightly.

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