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SUMMARY:Using orbits to probe ultra-light dark matter - Diego Blas (KCL)
DTSTART:20180521T120000Z
DTEND:20180521T130000Z
UID:TALK106276@talks.cam.ac.uk
CONTACT:Tobias Baldauf
DESCRIPTION:In this talk I will show how to use precision data from orbita
 l motion to constrain models of ultra-light dark matter (masses form 1E-22
  eV - 1E-18 eV). I will first discuss how these dark matter candidates aff
 ect pulsar timing observations (in particular in binary systems). Then\, I
  will describe the effect that the soliton that these models generate in t
 he center of galaxies has on orbital motions. As I will show\, these modif
 ications can be used to rule out some of the models.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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