Einstein's Theory of Gravity and the Problem of Missing Mass

被引:28
|
作者
Ferreira, Pedro G. [1 ]
Starkman, Glenn D. [2 ]
机构
[1] Univ Oxford, Dept Astrophys, Oxford OX2 7LG, England
[2] Case Western Reserve Univ, Dept Phys, Inst Sci Origins, Ctr Educ & Res Cosmol & Astrophys, Cleveland, OH 44106 USA
基金
英国科学技术设施理事会;
关键词
NEWTONIAN DYNAMICS; GALAXIES; MOND;
D O I
10.1126/science.1172245
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The observed matter in the universe accounts for just 5% of the observed gravity. A possible explanation is that Newton's and Einstein's theories of gravity fail where gravity is either weak or enhanced. The modified theory of Newtonian dynamics (MOND) reproduces, without dark matter, spiral-galaxy orbital motions and the relation between luminosity and rotation in galaxies, although not in clusters. Recent extensions of Einstein's theory are theoretically more complete. They inevitably include dark fields that seed structure growth, and they may explain recent weak lensing data. However, the presence of dark fields reduces calculability and comes at the expense of the original MOND premise, that the matter we see is the sole source of gravity. Observational tests of the relic radiation, weak lensing, and the growth of structure may distinguish modified gravity from dark matter.
引用
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页码:812 / 815
页数:4
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