Speaker
Daniel Phalen
(University of Michigan - Ann Arbor)
Description
Recently there have been many anomalies in the cosmic ray data in the energy range 10 GeV to 1 TeV. In addition, there is the WMAP "Haze" excess in the 22 GHz to 93 GHz frequency range. We propose that pulsars could describe all of these excesses and discuss the relevant astrophysics.
Primary author
Daniel Phalen
(University of Michigan - Ann Arbor)
