Dark matter phenomenology of high-speed galaxy cluster collisions

Abstract We perform a general computational analysis of possible post-collision mass distributions in high-speed galaxy cluster collisions in the presence of self-interacting dark matter. Using this analysis, we show that astrophysically weakly self-interacting dark matter can impart subtle yet meas...

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Bibliographic Details
Main Authors: Yuriy Mishchenko, Chueng-Ryong Ji
Format: Article
Language:English
Published: SpringerOpen 2017-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-5063-7

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