Perfil de materia oscura de grupos y cúmulos de galaxias: una aplicación del efecto lente gravitacional galaxia-galaxia
Published 2007-04-30
Keywords
- lentes gravitacionales,
- dark matter profiles,
- cosmology,
- power-spectrum
How to Cite
Abstract
Cosmology is in one of its most important periods of development. Theorical progress, and even more, growth in high-precision cosmological tests (satellites as WMAP and Planck) have given and will continue giving cosmology a period of unprecedented progress in the history of physics. The current paradigm of the so-called (ΛCDM) is supported so far, not without problems, by the general theory of relativity. However, two exotic components are dominant in current cosmological model: the dark matter and energy. We present one of the most direct and with fewer restrictions evidence on the study of fundamental cosmological parameters (Ωm, Ωλ, σ8 ) and analyze the use of shear in the cosmological study of the correlation function of two points. It is also briefly discussed the problem of bias among luminous matter and dark matter.
Keywords:lentes gravitacionales, dark matter profiles, cosmology, power-spectrum.
Downloads
References
[2] P. Schneider, J. Ehlers, E. Falco, Gravitational Lenses, Springer-Verlag: Heidelberg, 2nd printing, 1999 (SEF).
[3] P. Schneider, Weak Gravitational Lensing, astro-ph/0509252.
[4] T.G. Brainerd, R.D. Blandford, I. Smail, “Weak Gravitational Lensing by Galaxies”, Astrophysical Journal, 466, 623 (1996).