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- W3037005169 abstract "Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detection of various plausible baryonic candidates for dark matter inferred, e.g., from galaxy rotation curves and from cluster of galaxy velocity dispersions, the need for non-baryonic dark matter for theoretical models of galaxy formation, and the large discrepancy between dynamical measurements implying $Omega_0 > 0.2$ and the baryon abundance inferred from big bang nucleosynthesis, $Omega_b h^2 = 0.015$. There are a number of well-motivated dark matter candidates: massive neutrinos, supersymmetric dark matter and ``invisible'' axions. Many of these dark matter candidates are potentially detectable by the current generation of dark matter experiments." @default.
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- W3037005169 date "1997-01-01" @default.
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- W3037005169 title "Particle dark matter." @default.
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