Dark Matter or Regular Matter in Neutron Stars? How to tell the difference from the coalescence of compact objects
ORAL
Abstract
*H.T. and N.Y. acknowledge financial support through NSF grants No. PHY-1759615, PHY-1949838 and PHY-2207650. M.H. was supported in part by the National Science Foundation (NSF) within the framework of the MUSES collaboration, under grant number OAC-2103680. The research of DC was supported in part by a Discovery Grant from the Natural Sciences and Engineering Research Council of Canada, the Canada Research Chair program, the Alfred P. Sloan Foundation, the Ontario Early Researcher Award, and the University of Toronto McLean Award. J.N.H. acknowledges financial support by the US-DOE Nuclear Science Grant No. DESC0020633. E.D. acknowledges financial support from Internship Grant Funding – Berea College Internship Program. This material is based upon work supported by the National Science Foundation and the Department of Defense under Grant PHY-1950744. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily
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Presenters
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Hung Tan
- University of Illinois at Urbana-Champai