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• W2072031373 abstract "The possible relationships between phase transitions in the early universe and dark matter problems are discussed. It is shown that there are at least 3 distinct cosmological dark matter problems 1) halos; 2) galaxy formation and clustering; and 3) Ω = 1, each emphasizing different attributes for the dark matter. At least some of the dark matter must be baryonic but if problems 2 and 3 are real they seem to also require non-baryonic material. However, if seeds are generated at the quark-hadron-chiral symmetry transition then alternatives to the standard scenarios may occur. At present no simple simultaneous solution (neither “hot”, “warm”, nor “cold”) exists for all 3 problems, but non-standard solutions with strings, decaying particles or light not tracing to mass may work. An alternative interpretation of the relationship of the cluster-cluster and galaxy-galaxy correlation functions using renormalized scaling is mentioned. In this interpretation galaxies are more strongly correlated and the cluster-cluster function is not expected to go negative until ≳ 200 Mpc. Possible phase transition origins for the cluster-cluster renormalized scale are presented as ways to obtain a dimension 1.2 fractal." @default.
• W2072031373 created "2016-06-24" @default.
• W2072031373 creator A5077200443 @default.
• W2072031373 date "1985-01-01" @default.
• W2072031373 modified "2023-10-16" @default.
• W2072031373 title "Phase transitions and dark matter problems" @default.
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• W2072031373 doi "https://doi.org/10.1016/0550-3213(85)90425-0" @default.
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