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Shen, G; Meng, J; Hillhouse, GC; Shen, G , Peking Univ, Sch Phys, Beijing 100871, Peoples R China.
Direct URCA process in neutron stars
Source PublicationHIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
KeywordHalo
AbstractThe onset of the most powerful neutrino emission candidate in the cooling of neutron stars, direct URCA process, requires a high threshold proton fraction. The proton fraction in neutron stars relies on the isospin dependent part of nuclear force, which can be constrained by the measurement of the neutron skin thickness in heavy nuclei such as Pb-208. Adding new isospin dependent correction terms to the effective interactions PK1, NL3, S271 and Z271, the correlation between the proton fraction and neutron skin thickness in Pb-208 is studied. For a neutron star with fixed mass, the central proton fraction increases with increasing predicted values of neutron skin thickness in Pb-208.
2004
ISSN0254-3052
Volume28Issue:0Pages:99-101
Subject AreaPhysics
Indexed BySCI
Citation statistics
Document Type期刊论文
Identifierhttp://ir.itp.ac.cn/handle/311006/13943
Collection理论物理所科研产出_SCI论文
Corresponding AuthorShen, G , Peking Univ, Sch Phys, Beijing 100871, Peoples R China.
Recommended Citation
GB/T 7714
Shen, G,Meng, J,Hillhouse, GC,et al. Direct URCA process in neutron stars[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2004,28(0):99-101.
APA Shen, G,Meng, J,Hillhouse, GC,&Shen, G , Peking Univ, Sch Phys, Beijing 100871, Peoples R China..(2004).Direct URCA process in neutron stars.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,28(0),99-101.
MLA Shen, G,et al."Direct URCA process in neutron stars".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 28.0(2004):99-101.
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