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New orbitals probes of ultra-light dark matter

Research output: Contribution to journalArticlepeer-review

Original languageUndefined/Unknown
Pages (from-to)1845018
Number of pages1
JournalInternational Journal of Modern Physics A
Issue number34
Published1 Dec 2018

King's Authors


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).

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