Quenching of magnetic form factors of s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 within the relativistic mean field model

doi:10.1103/PhysRevC.92.014309

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	Quenching of magnetic form factors of s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 within the relativistic mean field model
	Wang, Zaijun 1; Ren, Zhongzhou 2,3; Dong, Tiekuang4 ; Guo, Xiaoyong 5
	2015-07-14
发表期刊	PHYSICAL REVIEW C
卷号	92 期号:1 页码:14309
摘要	The magnetic form factors of the odd-A s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 are studied within the relativistic frame with single-nucleon wave functions generated using the relativistic mean field model. Single valence-nucleon contributions to the nuclear magnetic form factors are calculated, and two sets of quenching ratios of the nuclear magnetic form factors relative to the single valence-nucleon contributions are extracted for each nucleus. It is found that the single valence-nucleon contributions can generally give a good approximate description for the shapes of the nuclear magnetic form factors, including the positions of the minima and maxima, and after the quenching ratios are applied the experimental data can be very well reproduced. The quenching ratios are compared with those obtained within some other nuclear models, and the physical implications for each nucleus are discussed. Calculations also show that no reasonable quenching ratios could be found for Al-27 when mu(expt.)/mu(s.n.) is chosen as the M1 multipole quenching ratio. This implies that the common way of choosing mu(expt.)/mu(s.n.) as the M1 multipole quenching ratio for the odd-A nuclei is not always valid.
文章类型	Article
WOS标题词	Science & Technology ; Physical Sciences
学科领域	天文和天体物理
DOI	10.1103/PhysRevC.92.014309
关键词[WOS]	ELASTIC ELECTRON-SCATTERING ; HARTREE-FOCK APPROACH ; CURRENT DENSITIES ; FINITE NUCLEI ; EXOTIC NUCLEI ; MOMENTS ; DISTRIBUTIONS ; RADIUS ; HALOS ; ORBIT
收录类别	SCI
语种	英语
资助项目	PMO_LIB-IR
WOS研究方向	Physics
WOS类目	Physics, Nuclear
WOS记录号	WOS:000357858700003
引用统计
文献类型	期刊论文
条目标识符	http://libir.pmo.ac.cn/handle/332002/14797
专题	暗物质和空间天文实验室
作者单位	1.Tianjin Univ Technol & Educ, Sch Sci, Tianjin 300222, Peoples R China 2.Nanjing Univ, Dept Phys, Nanjing 210008, Jiangsu, Peoples R China 3.Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China 4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 5.Tianjin Univ Sci & Technol, Sch Sci, Tianjin 300457, Peoples R China
推荐引用方式 GB/T 7714	Wang, Zaijun,Ren, Zhongzhou,Dong, Tiekuang,et al. Quenching of magnetic form factors of s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 within the relativistic mean field model[J]. PHYSICAL REVIEW C,2015,92(1):14309.
APA	Wang, Zaijun,Ren, Zhongzhou,Dong, Tiekuang,&Guo, Xiaoyong.(2015).Quenching of magnetic form factors of s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 within the relativistic mean field model.PHYSICAL REVIEW C,92(1),14309.
MLA	Wang, Zaijun,et al."Quenching of magnetic form factors of s-d shell nuclei O-17, Mg-25, Al-27, Si-29, and P-31 within the relativistic mean field model".PHYSICAL REVIEW C 92.1(2015):14309.

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