Review of Solutions to the Cusp-Core Problem of the ΛCDM Model

被引:22
作者
Del Popolo, Antonino [1 ,2 ]
Le Delliou, Morgan [3 ,4 ,5 ]
机构
[1] Univ Catania, Dipartimento Fis & Astron, Viale Andrea Doria 6, I-95125 Catania, Italy
[2] Russian Acad Sci, Inst Astron, Pyatnitskaya Str 48, Moscow 119017, Russia
[3] Lanzhou Univ, Inst Theoret Phys, Sch Phys Sci & Technol, 222 South Tianshui Rd, Lanzhou 730000, Peoples R China
[4] Univ Lisbon, Inst Astrofis & Ciencias Espaco, Fac Ciencias, Ed C8, P-1769016 Lisbon, Portugal
[5] Lanzhou Univ, Lanzhou Ctr Theoret Phys, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China
来源
GALAXIES | 2021年 / 9卷 / 04期
基金
美国国家科学基金会;
关键词
cosmology; dark matter; cusp-core problem; CDM model; COLD DARK-MATTER; MICROWAVE-ANISOTROPY-PROBE; HIGH-RESOLUTION MEASUREMENTS; SURFACE BRIGHTNESS GALAXIES; DWARF SPHEROIDAL GALAXIES; CONSTANT-DENSITY CORES; DYNAMICAL FRICTION; HIGH-REDSHIFT; HALO MASS; COSMOLOGICAL SIMULATIONS;
D O I
10.3390/galaxies9040123
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This review aims at proposing to the field an overview of the Cusp-core problem, including a discussion of its advocated solutions, assessing how each can satisfactorily provide a description of central densities. Whether the Cusp-core problem reflects our insufficient grasp on the nature of dark matter, of gravity, on the impact of baryonic interactions with dark matter at those scales, as included in semi-analytical models or fully numerical codes, the solutions to it can point either to the need for a paradigm change in cosmology, or to to our lack of success in ironing out the finer details of the ? CDM paradigm.
引用
收藏
页数:33
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