How cold dark matter theory explains Milgrom's law

被引:52
作者
Kaplinghat, M
Turner, M
机构
[1] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[2] Fermilab Natl Accelerator Lab, NASA, Fermilab Astrophys Ctr, Batavia, IL 60510 USA
[3] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 USA
关键词
dark matter; galaxies : fundamental parameters galaxies : halos; galaxies : kinematics and dynamics galaxies : spiral; gravitation;
D O I
10.1086/340578
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Milgrom noticed the remarkable fact that the gravitational effect of dark matter in galaxies only becomes important where accelerations are less than about 10(-8) cm s(-2) similar to cH(o) ("Milgrom's law"). This forms the basis for modified Newtonian dynamics, an alternative to particle dark matter. However, any successful theory of galactic dynamics must account for Milgrom's law. We show how Milgrom's law comes about in the cold dark matter theory of structure formation.
引用
收藏
页码:L19 / L22
页数:4
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