Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-01-27
Nature 433 (2005) 389-391
Astronomy and Astrophysics
Astrophysics
11 pages, 3 figures, published in Nature, January 27, 2005
Scientific paper
10.1038/nature03270
The Universe was nearly smooth and homogeneous before a redshift of z = 100, about 20 million years after the Big Bang. After this epoch, the tiny fluctuations imprinted upon the matter distribution during the initial expansion began to collapse because of gravity. The properties of these fluctuations depend on the unknown nature of dark matter, the determination of which is one of the biggest challenges in present-day science. Here we report supercomputer simulations of the concordance cosmological model, which assumes neutralino dark matter (at present the preferred candidate), and find that the first objects to form are numerous Earth-mass dark-matter haloes about as large as the Solar System. They are stable against gravitational disruption, even within the central regions of the Milky Way. We expect over 10^15 to survive within the Galactic halo, with one passing through the Solar System every few thousand years. The nearest structures should be among the brightest sources of gamma-rays (from particle-particle annihilation).
Diemand Juerg
Moore Ben
Stadel Joachim
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