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	Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model
	Wang, Xu Dong; Qi, Bin; Yang, Gao Le; Zhang, Nai Bo
刊名	INTERNATIONAL JOURNAL OF MODERN PHYSICS D
	2019
卷号	28期号:11
关键词	Neutron stars dark matter relativistic mean field theory weakly interacting massive particles
DOI	10.1142/S0218271819501487
URL标识	查看原文
公开日期	[db:dc_date_available]
内容类型	期刊论文
URI标识	http://www.corc.org.cn/handle/1471x/4551821
专题	山东大学
作者单位	Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Sch Space Sci & Phys, Inst Spa
推荐引用方式 GB/T 7714	Wang, Xu Dong,Qi, Bin,Yang, Gao Le,et al. Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2019,28(11).
APA	Wang, Xu Dong,Qi, Bin,Yang, Gao Le,&Zhang, Nai Bo.(2019).Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,28(11).
MLA	Wang, Xu Dong,et al."Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 28.11(2019).

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