Dark matter and dark matter candidates

Keith A. Olive

doi:10.1016/j.asr.2007.07.040

Dark matter and dark matter candidates

Keith A. Olive

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

The nature and identity of the dark matter of the Universe is one of the most challenging problems facing modern cosmology. Only 5% of the energy density of the Universe can be associated with known forms of matter. Problems for baryonic and neutrino dark matter imply the necessity to search beyond the standard model for dark matter candidates. Emphasis is placed on the prospects for supersymmetric dark matter.

Original language	English (US)
Pages (from-to)	581-590
Number of pages	10
Journal	Advances in Space Research
Volume	42
Issue number	3
DOIs	https://doi.org/10.1016/j.asr.2007.07.040
State	Published - Aug 5 2008

Bibliographical note

Funding Information:
This work was supported in part by DOE Grant DE-FG02-94ER-40823.

Keywords

Cosmology
Dark matter

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10.1016/j.asr.2007.07.040

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abstract = "The nature and identity of the dark matter of the Universe is one of the most challenging problems facing modern cosmology. Only 5% of the energy density of the Universe can be associated with known forms of matter. Problems for baryonic and neutrino dark matter imply the necessity to search beyond the standard model for dark matter candidates. Emphasis is placed on the prospects for supersymmetric dark matter.",

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AB - The nature and identity of the dark matter of the Universe is one of the most challenging problems facing modern cosmology. Only 5% of the energy density of the Universe can be associated with known forms of matter. Problems for baryonic and neutrino dark matter imply the necessity to search beyond the standard model for dark matter candidates. Emphasis is placed on the prospects for supersymmetric dark matter.

KW - Cosmology

KW - Dark matter

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Dark matter and dark matter candidates

Abstract

Bibliographical note

Keywords

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