New orbitals probes of ultra-light dark matter

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Abstract

I will discuss how to use precision data from orbital motion of binary pulsars to constrain models of ultra-light dark matter (masses in the range 10−21 eV to 10−18 eV).
Original languageEnglish
JournalInternational Journal of Modern Physics A
DOIs
Publication statusPublished - 1 Dec 2018

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