# Dark Matter

@inproceedings{Zacek2007DarkM,
title={Dark Matter},
author={Viktor Zacek},
year={2007}
}
The nature of the main constituents of the mass of the universe is one of the outstanding riddles of cosmology and astro-particle physics. Current models explaining the evolution of the universe, and measurements of the various components of its mass, all have in common that an appreciable contribution to that mass is non-luminous and non-baryonic, and that a large fraction of this so-called dark matter must be in the form of non-relativistic massive particles (Cold Dark Matter: CDM). In the…

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## References

SHOWING 1-10 OF 26 REFERENCES
The early Universe
• Physics, Education
Nature
• 1981
In the past few years one of the most exciting areas of research in physics has been the interdisciplinary field of cosmology and particle physics. The NSF's Institute for Theoretical Physics in
The Search for the Dark Matter: WIMPs and MACHOs
• K. Griest
• Physics
Annals of the New York Academy of Sciences
• 1993
The status of experiments and ideas relevant for the detection of the dark matter, which is suspected to be the dominant constituent of the Universe, are reviewed.
The New Scientist
In addition to its own weight, it will carry a 32 kilogram payload within the backpack. To the pilot this would feel like they were carrying just 2 kilograms, says Kazerooni. All the best science
Phys.Lett. B621
• Phys.Lett. B621
• 2005
Proc. of the 6 th Inter. Conf. on the Identification of Dark Matter
• Proc. of the 6 th Inter. Conf. on the Identification of Dark Matter
• 2006
Proc. of the 7 th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy
• Proc. of the 7 th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy
• 2006
phys. J. S
• phys. J. S
• 2003
A. phys. J
• A. phys. J
• 2005
Phys. Rev. D
• Phys. Rev. D
• 2004