Abstract
A new method for deriving a lower limit of the mean density of the universe using the maximum temperature of the X-ray-emitting hot gas in clusters of galaxies is proposed. This method is applied to the present record holder for the highest temperature among X-ray clusters, A2163. I find that the probability that the observed volume, in which complete X-ray observations are performed, contains at least one cluster with a temperature as high as the temperature of A2163 is very small for a low-density universe. Even if we take the most conservative upper limit of the baryon density of the universe derived from big bang primordial nucleo-synthesis theories, the possibility that the universe is made from only baryonic matter can be rejected with more than 99.99% confidence. Applying the condition that the expectation of finding a cluster which has a temperature higher than A2163 in the observed volume is at least 1, the mean density of the universe must be more than twice the baryon density of the universe. I conclude that it is very probable that our universe is gravitationally dominated by non-baryonic dark matter.
Original language | English |
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Pages (from-to) | 19-22 |
Number of pages | 4 |
Journal | Astrophysical Journal |
Volume | 426 |
Issue number | 1 |
DOIs | |
Publication status | Published - 1994 May 1 |
Externally published | Yes |
Keywords
- Cosmology: dark matter
- Galaxies: clustering
- X-rays: galaxies
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science