中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 近代物理研究所
  3. 中国科学院近代物理研究所
Dark compact objects: An extensive overview

文献类型：期刊论文

作者Deliyergiyev, Maksym5,6; Del Popolo, Antonino2,3,4; Tolos, Laura1,9,10,11; Le Delliou, Morgan7,8; Lee, Xiguo2; Burgio, Fiorella3
刊名PHYSICAL REVIEW D
出版日期2019-03-22
卷号99期号:6页码:17
ISSN号2470-0010
DOI10.1103/PhysRevD.99.063015
通讯作者Le Delliou, Morgan(delliou@lzu.edu.cn)
英文摘要We study the structure of compact objects that contain non-self annihilating, self-interacting dark matter admixed with ordinary matter made of neutron star and white dwarf materials. We extend the previous work [Phys. Rev. D 92, 123002 (2015)] on these dark compact objects by analyzing the effect of weak and strongly interacting dark matter with particle masses in the range of 1-500 GeV, so as to set some constraints in the strength of the interaction and the mass of the dark matter particle. We find that the total mass of the compact objects increases with decreasing dark matter particle mass. In the strong interacting case and for dark matter particle masses in the range 1-10 GeV, the total mass of the compact objects largely exceeds the 2 M-circle dot constraint for neutron star masses and the nominal 1 M-circle dot for white dwarfs, while for larger dark matter particle masses or in the weakly interacting case the compact objects show masses in agreement or smaller than these constraints, thus hinting at the exclusion of strongly self-interacting dark matter of masses 1-10 GeV in the interior of these compact objects. Moreover, we observe that the smaller the dark matter particle mass, the larger the quantity of dark matter captured is, putting constraints on the dark matter mass trapped in the compact objects so as to fulfill similar or equal to 2 M-circle dot observations. Finally, the inhomogeneity of distribution of dark matter in the Galaxy implies a mass dependence of compact objects from the environment which can be used to put constraints on the characteristics of the Galaxy halo DM profile and on particle mass. In view of these results, we discuss the formation of the dark compact objects in an homogeneous and nonhomogeneous dark matter environment.
WOS关键词NEUTRON-STARS ; OBSERVATIONAL EVIDENCE ; 3RD FAMILY ; MATTER ; PARTICLE ; UNIVERSE ; SEARCH ; DENSE
资助项目Chinese Academy of Sciences Presidents International Fellowship Initiative[2016PM043] ; Polish National Science Centre (NCN)[2016/23/B/ST2/00692] ; Lanzhou University starting fund ; Heisenberg Programme of the Deutsche Forschungsgemeinschaft[383452331] ; PHAROS COST Action[CA16214] ; Ministerio de Ciencia, Innovacion y Universidades[FPA2016-81114-P]
WOS研究方向Astronomy & Astrophysics ; Physics
语种英语
WOS记录号WOS:000462916500002
出版者AMER PHYSICAL SOC
资助机构Chinese Academy of Sciences Presidents International Fellowship Initiative ; Polish National Science Centre (NCN) ; Lanzhou University starting fund ; Heisenberg Programme of the Deutsche Forschungsgemeinschaft ; PHAROS COST Action ; Ministerio de Ciencia, Innovacion y Universidades
源URL[http://119.78.100.186/handle/113462/134169]  
专题中国科学院近代物理研究所
通讯作者Le Delliou, Morgan
作者单位1.Goethe Univ Frankfurt, Inst Theoret Phys, Max von Laue Str 1, D-60438 Frankfurt, Germany
2.Chinese Acad Sci, Inst Modern Phys, POB 31, Lanzhou 730000, Gansu, Peoples R China
3.Ist Nazl Fis Nucl, Sez Catania, Via S Sofia 64, I-95123 Catania, Italy
4.Univ Catania, Dipartimento Fis & Astron, Viale Andrea Doria 6, I-95125 Catania, Italy
5.Jan Kochanowski Univ Humanities & Sci, Inst Phys, PL-25406 Kielce, Poland
6.Chinese Acad Sci, Inst Modern Phys, Dept High Energy Nucl Phys, POB 31, Lanzhou 730000, Gansu, Peoples R China
7.Univ Lisbon, Inst Astrofis & Ciencias Espaco, Fac Ciencias, Ed C8, P-1769016 Lisbon, Portugal
8.Lanzhou Univ, Inst Theoret Phys, Phys Dept, 222 South Tianshui Rd, Lanzhou 730000, Gansu, Peoples R China
9.IEEC, Barcelona 08034, Spain
10.CSIC, Inst Space Sci ICE, Campus UAB, Barcelona 08193, Spain
推荐引用方式
GB/T 7714		 Deliyergiyev, Maksym,Del Popolo, Antonino,Tolos, Laura,et al. Dark compact objects: An extensive overview[J]. PHYSICAL REVIEW D,2019,99(6):17.
APA Deliyergiyev, Maksym,Del Popolo, Antonino,Tolos, Laura,Le Delliou, Morgan,Lee, Xiguo,&Burgio, Fiorella.(2019).Dark compact objects: An extensive overview.PHYSICAL REVIEW D,99(6),17.
MLA Deliyergiyev, Maksym,et al."Dark compact objects: An extensive overview".PHYSICAL REVIEW D 99.6(2019):17.

入库方式： OAI收割

来源：近代物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。