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arXiv · 1802.01005

The leptophilic dark matter in the Sun: the minimum testable mass

Zheng-Liang Liang·Yi-Lei Tang·Zi-Qing Yang
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Abstract

The physics of the solar dark matter (DM) that are captured and thermalise through the DM-nucleon interaction has been extensively studied. In this work, we consider the leptophilic DM scenario where the DM particles interact exclusively with the electrons through the axial-vector coupling. We investigate relevant phenomenologies in the Sun, including its capture, evaporation and thermalisation, and we calculate the equilibrium distribution using the Monte Carlo methods, rather than adopting a semi-analytic approximation. Based on the analysis, we then determine the minimum testable mass for which the DM-electron coupling strength can be probed via the neutrino observation. Compared to the case of the DM-nucleon interaction, it turns out that minimum detectable mass of the DM-electron interaction is roughly 1 GeV smaller, and a cross section about two orders of magnitude larger is required for the saturation of the annihilation signal.

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Zheng-Liang Liang, Yi-Lei Tang, Zi-Qing Yang. 2018-10-11. The leptophilic dark matter in the Sun: the minimum testable mass. https://doi.org/10.1088/1475-7516%2F2018%2F10%2F035

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