Research ArticleOpen AccessGoogle Scholar indexed
A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
Universidad San Francisco de Quito, Quito, Ecuador
- 1 Universidad San Francisco de Quito, Quito, Ecuador
International Journal of Astronomy and Astrophysics·Volume 13 (2023)·Pages 25–38·Published 17 March 2023·DOI10.4236/ijaa.2023.131002
Copy link · social · email
Abstract
In the warm dark matter scenario, the Press-Schechter formalism is valid only for galaxy masses greater than the “velocity dispersion cut-off”. In this work we extend the predictions to masses below the velocity dispersion cut-off, and thereby address the “Missing Satellites Problem” of the cold dark matter ΛCDM scenario, and the rest-frame ultra-violet luminosity cut-off required to not exceed the measured reionization optical depth. For warm dark matter we find agreement between predictions and observations of these two phenomena. As a by-product, we obtain the empirical Tully-Fisher relation from first principles.
KeywordsCosmology: Dark MatterGalaxies: Statistics
- Klypin, A.A., Kravstov, A.V. and Valenzuela, O. (1999) Where Are the Missing Galactic Satellites? The Astrophysical Journal, 522, 82-92. https://doi.org/10.1086/307643
- Aghanim, N., et al. (2018) Planck 2018 Results. VI. Cosmological Parameters. Astronomy & Astrophysics, 641, A6.
- Workman, R.L., et al. (Particle Data Group) (2022) The Review of Particle Physics. Progress of Theoretical and Experimental Physics, 2022, 083C01.
- Lapi, A. and Danese, L. (2015) Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck. Journal of Cosmology and Astroparticle Physics, 9, 3. https://doi.org/10.1088/1475-7516/2015/09/003
- Mason, C.A., Trenti, M. and Treu, T. (2015) The Galaxy UV Luminosity Function before the Epoch of Reionization. The Astrophysical Journal, 813, 21. https://doi.org/10.1088/0004-637X/813/1/21
- Hoeneisen, B. (2022) Measurement of the Dark Matter Velocity Dispersion with Galaxy Stellar Masses, UV Luminosities, and Reionization. International Journal of Astronomy and Astrophysics, 12, 258-272. https://doi.org/10.4236/ijaa.2022.123015
- Press, W.H. and Schechter, P. (1974) Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation. The Astrophysical Journal, 187, 425-438. https://doi.org/10.1086/152650
- Sheth, R.K. and Tormen, G. (1999) Large-Scale Bias and the Peak Background Split. Monthly Notices of the Royal Astronomical Society, 308, 119-126. https://doi.org/10.1046/j.1365-8711.1999.02692.x
- Sheth, R.K., Mo, H.J. and Tormen, G. (2001) Ellipsoidal Collapse and an Improved Model for the Number and Spatial Distribution of Dark Matter Haloes. Monthly Notices of the Royal Astronomical Society, 323, 1-12. https://doi.org/10.1046/j.1365-8711.2001.04006.x
- Lapi, A., et al. (2017) Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation. The Astrophysical Journal, 847, 13. https://doi.org/10.3847/1538-4357/aa88c9
- Song, M., Finkelstein, S.L., Ashby, M.L.N., et al. (2016) The Evolution of the Galaxy Stellar Mass Function at z = 4-8: A Steepening Low-Mass-End Slope with Increasing Redshift. The Astrophysical Journal, 825, 5. https://doi.org/10.3847/0004-637X/825/1/5
- Grazian, A., Fontana, A., Santini, P., et al. (2015) The Galaxy Stellar Mass Function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF Fields. Astronomy and Astrophysics, 575, A96. https://doi.org/10.1051/0004-6361/201424750