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Sterile neutrino dark matter is expected to suppress structure formation at small astrophysical scales.
A. A. Klypin, A. V. Kravtsov, O. Valenzuela and F. Prada, “Where are the missing Galactic satellites?,” Astrophys. J. 522
1999
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B. Moore, S. Ghigna, F. Governato, G. Lake, T. R. Quinn, J. Stadel and P. Tozzi, “Dark matter substructure within galactic halos,” Astrophys. J. 524
1999
Earlier work this paper cites.
X. D. Shi and G. M. Fuller, “A New dark matter candidate: Nonthermal sterile neutrinos,” Phys. Rev. Lett. 82
1999
Earlier work this paper cites.
A. Kusenko, “Sterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet,” Phys. Rev. Lett. 97
2006
Earlier work this paper cites.
M. Shaposhnikov and I. Tkachev, “The nuMSM, inflation, and dark matter,” Phys. Lett. B 639
2006
Cited alongside, same era.
W. J. G. de Blok, “The Core-Cusp Problem,” Adv. Astron. 2010
2010
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2013
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2015
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Cited in the paper.
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Cited in the paper.
2015
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2016
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2016
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2016
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