New constraint on massive degenerate neutrinos from big-bang nucleosynthesis and cosmic microwave background fluctuations

被引:0
|
作者
Kajino, T [1 ]
Orito, M [1 ]
Ichiki, K [1 ]
Mathews, GJ [1 ]
机构
[1] Natl Astron Observ, Div Theoret Astrophys, Mitaka, Tokyo 1818588, Japan
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose two cosmological models in order to explain the universal baryon density parameter Omega(b)h(2) inferred from different observational data: One is from the Big-Bang nucleosynthesis, and the other is from the cosmic microwave background fluctuations. Our proposed theoretical models axe the lepton asymmetric Universe model and the baryon inhomogeneous Big-Bang nucleosynthesis model.
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页码:435 / 440
页数:6
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