Articles Citing

Dwarf Galaxies Imply Dark Matter Is Heavier than $2.2 \times 10^{- 21} eV$

Tim Zimmermann ^1,*, James Alvey ^2,3,4,†, David J. E. Marsh ^5,‡, Malcolm Fairbairn ^5,§, and Justin I. Read^6,∥

¹Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, Oslo, Norway
²Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
³Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
⁴GRAPPA Institute, Institute for Theoretical Physics Amsterdam, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands
⁵Theoretical Particle Physics and Cosmology, King’s College London, Strand, London WC2R 2LS, United Kingdom
⁶Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom

^*Contact author: timzi@astro.uio.no
^†Contact author: jbga2@cam.ac.uk
^‡Contact author: david.j.marsh@kcl.ac.uk
^§Contact author: malcolm.fairbairn@kcl.ac.uk
^∥Contact author: j.read@surrey.ac.uk

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Articles Citing

Dwarf Galaxies Imply Dark Matter Is Heavier than $2.2 \times 10^{- 21} eV$

Dark matter

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Ultralight dark matter simulations and stellar dynamics: Tension in dwarf galaxies for m<5×10−21 eV

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Detecting dark matter substructure with lensed quasars in optical bands

Mass modelling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII

Fuzzy axions and associated relics

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