Varying leptonic chemical potentials and spatial variation of primordial deuterium at high z

被引:14
作者
Dolgov, AD
Pagel, BEJ
机构
[1] Teoret Astrofys Ctr, DK-2100 Copenhagen, Denmark
[2] NORDITA, DK-2100 Copenhagen, Denmark
[3] ITEP, Moscow 113259, Russia
来源
NEW ASTRONOMY | 1999年 / 4卷 / 04期
关键词
early universe; cosmic microwave background; ISM : abundances; galaxies : abundances; quasars : absorption lines;
D O I
10.1016/S1384-1076(99)00007-X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We try to explain the spatial variation of primordial deuterium suggested by some observations by varying leptonic chemical potentials. The variation of the latter may take place in some scenarios of leptogenesis. The model predicts a large mass fraction of He-4 (35-60%) and Li-7 (up to 10(-9)) in deuterium-rich regions. Because of lepton family symmetry, the angular variations of cosmic microwave background radiation can be sufficiently small although still observable in future measurements. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:223 / 230
页数:8
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