The dark matter problem from f(R) gravity viewpoint

被引:196
作者
Capozziello, Salvatore [1 ,2 ]
De Laurentis, Mariafelicia [2 ]
机构
[1] Univ Naples Federico II, Dipartimento Sci Fis, I-80126 Naples, Italy
[2] INFN Sez Napoli, I-80126 Naples, Italy
关键词
DM; alternative theories of gravity; self-gravitating systems; HUBBLE-SPACE-TELESCOPE; ELLIPTIC GALAXY SURVEY; SKY SURVEY DATA; COSMOLOGICAL CONSTANT; EXTENDED THEORIES; NEWTONIAN LIMIT; DENSITY PROFILE; REDSHIFT SURVEY; POWER-SPECTRUM; MILKY-WAY;
D O I
10.1002/andp.201200109
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
An alternative view to the dark matter puzzle is represented by Extended Theories of Gravity. The approach consists in addressing issues like dark components from the point of view of gravitational field instead of requiring new material ingredients that, up to now, have not been detected at fundamental level. In this review paper, by extending the Hilbert-Einstein action of gravitational field to more general actions (e.g. f(R) gravity), it is shown that several gravitating structures like stars, spiral galaxies, elliptical galaxies and clusters of galaxies can be self-consistently described without asking for dark matter. It is also shown that standard General Relativity tests and Equivalence Principle constraints can be evaded at Solar System scales.
引用
收藏
页码:545 / 578
页数:34
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