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Similarly to warm dark matter which features a cut-off in the matter power spectrum due to free-streaming, many interacting dark matter models predict a suppression of the matter power spectrum on small length scales through collisional damping.
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1903
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2001
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2001
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2001
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2001
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2001
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2002
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A.D. Dolgov and S.H. Hansen, Massive sterile neutrinos as warm dark matter
2002
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Xue-lei Chen, Steen Hannestad, and Robert J. Scherrer, Cosmic microwave background and large scale structure limits on the interaction between dark matter and baryons
2002
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Celine Boehm, Alain Riazuelo, Steen H. Hansen, and Richard Schaeffer, Interacting dark matter disguised as warm dark matter
2002
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2003
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Maxim Markevitch, A. H. Gonzalez, D. Clowe, et al., Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56
2004
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Matias Zaldarriaga, Steven R. Furlanetto, and Lars Hernquist, 21 Centimeter fluctuations from cosmic gas at high redshifts
2004
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Takehiko Asaka, Steve Blanchet, and Mikhail Shaposhnikov, The nuMSM, dark matter and neutrino masses
2005
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2005
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2005
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2006
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2006
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2007
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Celine Boehm, Yasaman Farzan, Thomas Hambye, Sergio Palomares-Ruiz, and Silvia Pascoli, Is it possible to explain neutrino masses with scalar dark matter?
2008
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2009
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2009
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2015
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2015
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2010
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David E. Kaplan, Gordan Z. Krnjaic, Keith R. Rehermann, and Christopher M. Wells, Atomic Dark Matter
2010
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2010
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2010
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2011
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2011
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2017
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2017
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P. Ko, Natsumi Nagata, and Yong Tang, Hidden Charged Dark Matter and Chiral Dark Radiation
2017
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2017
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2017
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David R. DeBoer et al., Hydrogen Epoch of Reionization Array (HERA)
2017
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2017
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2018
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2018
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Sean Fraser et al., The EDGES 21 cm Anomaly and Properties of Dark Matter
2018
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2018
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2019
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Julia Stadler, Celine Bœhm, and Olga Mena, Is it Mixed dark matter or neutrino masses?
2020
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A. Weltman et al., Fundamental physics with the Square Kilometre Array
2020
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