CAS OpenIR  > 中科院上海原子核所2003年前
Temperature dependence of the proton fraction in hot neutron stars
Chen, LW; Zhang, FS; Lu, ZH; Li, WF; Zhu, ZY(朱志远); Ma, HR
2001
Source PublicationJOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
ISSN0954-3899
Volume27Issue:8Pages:1799
AbstractTemperature dependence of the proton fraction in beta -stable hot neutron stars matter is investigated within the framework of the Skyrme-Hartree-Fock theory using the extended Skyrme effective interaction. It is found that the proton fraction decreases with increasing temperature. This phenomenon is determined mainly by the temperature dependence of the nuclear matter symmetry energy within the present theoretical framework.
Indexed BySCI
Language英语
Funding Project应物所项目组
WOS IDWOS:000170694200012
Citation statistics
Cited Times:15[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/10210
Collection中科院上海原子核所2003年前
Recommended Citation
GB/T 7714
Chen, LW,Zhang, FS,Lu, ZH,et al. Temperature dependence of the proton fraction in hot neutron stars[J]. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,2001,27(8):1799.
APA Chen, LW,Zhang, FS,Lu, ZH,Li, WF,Zhu, ZY,&Ma, HR.(2001).Temperature dependence of the proton fraction in hot neutron stars.JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,27(8),1799.
MLA Chen, LW,et al."Temperature dependence of the proton fraction in hot neutron stars".JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 27.8(2001):1799.
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