17-22 July 2016
Master Cutlers Hall
Europe/London timezone

Latest status of the 3.5 keV line as a Dark Matter candidate

20 Jul 2016, 12:00
20m
Venue: Cutlers' Main Hall (First Floor); Chair: Paolo Gorla; Session Managers: David Woodward & Anthony Ezeribe ()

Venue: Cutlers' Main Hall (First Floor); Chair: Paolo Gorla; Session Managers: David Woodward & Anthony Ezeribe

Speaker

Mr. Jeroen Franse (Leiden University)

Description

The unidentified emission line from galaxies and cluster at 3.5 keV discovered in 2014 remains an interesting candidate for a dark matter decay signal. I will briefly review the existing work and arguments, and then present and discuss the current status of this signal and the latest results, such as the studies of the Draco satellite galaxy and the Perseus galaxy cluster.

Primary author

Mr. Jeroen Franse (Leiden University)

Presentation Materials

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