Thermal transport of the solar captured dark matter and its implication

Chian Shu Chen, Guey Lin Lin, Yen Hsun Lin

研究成果: Conference article

摘要

We study the thermal transport occurring in the system of solar captured dark matter (DM) and explore its impact on the DM indirect search signal. We particularly focus on the scenario of self-interacting DM (SIDM). We examine the DM temperature evolution and demonstrate that the DM temperature can be higher than the core temperature of the Sun. such that the energy flow due to DM self-interaction becomes relatively important. We argue that the correct DM temperature should be used for accurately predicting the DM annihilation rate, which is relevant to the DM indirect detection.

原文English
文章編號385
期刊Proceedings of Science
22-29-July-2015
出版狀態Published - 2015 一月 1
事件23rd European Physical Society Conference on High Energy Physics, EPS-HEP 2015 - Vienna, Austria
持續時間: 2015 七月 222015 七月 29

指紋

dark matter
temperature

All Science Journal Classification (ASJC) codes

  • General

引用此文

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Thermal transport of the solar captured dark matter and its implication. / Chen, Chian Shu; Lin, Guey Lin; Lin, Yen Hsun.

於: Proceedings of Science, 卷 22-29-July-2015, 385, 01.01.2015.

研究成果: Conference article

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