Halo mass function
In cosmology, the halo mass function is a mass distribution of dark matter halos. Specifically, it gives the number density of dark matter halos per mass interval.[1]
See also
References
- ^ Wu, Hao-Yi; Zentner, Andrew R.; Wechsler, Risa H. (2010-04-20). "The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology". The Astrophysical Journal. 713 (2): 856–864. arXiv:0910.3668. Bibcode:2010ApJ...713..856W. doi:10.1088/0004-637X/713/2/856.
External links
- Halo Mass Functions on the NMSU website
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Dark matter
dark matter
- Baryonic dark matter
- Cold dark matter
- Hot dark matter
- Light dark matter
- Mixed dark matter
- Warm dark matter
- Self-interacting dark matter
- Scalar field dark matter
- Primordial black holes
- Axino
- Axion
- Dark photon
- LSP
- Minicharged particle
- Neutralino
- Sterile neutrino
- SIMP
- WIMP
- WISP
and objects
- Cuspy halo problem
- Dark fluid
- Dark galaxy
- Dark globular cluster
- Dark matter halo
- Dark radiation
- Dark star
- Dwarf galaxy problem
- Halo mass function
- Mass dimension one fermions
- Massive compact halo object
- Mirror matter
- Navarro–Frenk–White profile
- Scalar field dark matter
experiments
| Direct detection | |
|---|---|
| Indirect detection | |
| Other projects |
Category
Commons
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