New orbitals probes of ultra-light dark matter

Research output: Contribution to journalArticlepeer-review

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 languageUndefined/Unknown
Pages (from-to)1845018
Number of pages1
JournalInternational Journal of Modern Physics A
Volume33
Issue number34
DOIs
Publication statusPublished - 1 Dec 2018

Keywords

  • Light dark matter, binary pulsars, 95.35.+d, 97.60.Gb, Dark matter, Pulsars

Cite this