NON-STANDARD BARYON-DARK MATTER INTERACTIONS

被引:1
|
作者
Famaey, B. [1 ]
Bruneton, J. -P. [2 ,3 ]
机构
[1] Univ Libre Bruxelles, IAA, Bvd Triomphe, B-1050 Brussels, Belgium
[2] ISAS, SISSA, I-34014 Trieste, Italy
[3] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
关键词
Gravitation; dark matter; MODIFIED NEWTONIAN DYNAMICS; MASS; MOND; GALAXIES;
D O I
10.1142/9789814293792_0026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
After summarizing the respective merits of the Cold Dark Matter (CDM) and Modified Newtonian Dynamics (MOND) paradigms in various stellar systems, we investigate the possibility that a non-standard interaction between baryonic matter and dark matter could reproduce the successes of CDM at extragalactic scales while making baryonic matter effectively obey the MOND field equation in spiral galaxies.
引用
收藏
页码:335 / +
页数:2
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