Constraining dark matter with neutron stars
ORAL
Abstract
I will discuss some recent theoretical developments that allow us to use multi-messenger observations of neutron stars to constrain the properties of candidate dark matter particles with masses less than about a GeV.
*My work was supported by the U.S. DOE under Grants No. DE-FG02- 00ER41132 and in part by the National Science Foundation Grant No. PHY- 1430152 (JINA Center for the Evolution of the Elements).
–
Presenters
-
Sanjay Kumar Reddy
- Univ of Washington