Fuzzy cold dark matter: the wave properties of ultralight particles.
By Wayne Hu, R. Barkana, A. Gruzinov. Physical Review Letters, 2000
965 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/81d1198aa1bcdcce551ef4d74aa0e26fe46ee98a
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In Astronomy and Astrophysics
- Volker Springel
- L. Hernquist
- P. Hopkins
- H. Hoekstra
- Simon D. M. White
- Lavinia Heisenberg
- D. Marsh
- M. Vogelsberger
In Nuclear and High Energy Physics
- Lavinia Heisenberg
- D. Marsh
- Florian Kuhnel
- Tomi Koivisto
- C. Yéche
- N. Palanque-Delabrouille
- B. Carr
- S. Tsujikawa
Citations in the corpus
- Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter (2017, methodology): “These effects are caused by the integrated effect on the expansion rate (when wa ≈−1, axions behave as DE), and the axion Jeans scale (axions do not cluster for k> kJ) (Hu et al. 2000; Arvanitaki et al. 2010; Hložek et al. 2015; Marsh 2016).”
- Constraining the mass of light bosonic dark matter using SDSS Lyman-α forest (2017, methodology): “…for several values of ma in the range 10−23 − 10−20 eV, we find the following scaling relation for the cutoff mode kc defined by T(kc) = 0.5 : kc = 4.97 ( ma 10−22 eV )0.46 Mpc−1 (7) This relation is in good agreement with those found MNRAS 000, 1–11 (2017) in Hu et al. (2000); Marsh & Silk (2014).”
- Flat central density profiles from scalar field dark matter halos (2003, background): “Furthermore, it has been shown previously that dark halos of galaxies could be scalar solitonic objects, even in the presence of baryonic matter, Hu et al 2000; Lee and Koh 1996; Arbey et al 2001, 2002; Sin 1994; and Ji and Sin 1994.”
- ETHOS - an effective theory of structure formation: dark matter physics as a possible explanation of the small-scale CDM problems (2015, background): “To mention a couple of less explored models, DM from late decays (Sigurdson & Kamionkowski 2004; Kaplinghat 2005; Borzumati et al. 2008), and extremely light DM forming condensates (Hu et al. 2000; Peebles 2000) with particle masses of the order of 10−22eV.”