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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, Zaijun1; Ren, Zhongzhou2,3; Dong, Tiekuang4 ; Guo, Xiaoyong5
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| 2015-07-14 | |
| Source Publication | PHYSICAL REVIEW C
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| Volume | 92Issue:1Pages:14309 |
| Abstract | 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. |
| Subject Area | 天文和天体物理 |
| WOS Headings | Science & Technology ; Physical Sciences |
| DOI | 10.1103/PhysRevC.92.014309 |
| WOS Keyword | ELASTIC ELECTRON-SCATTERING ; HARTREE-FOCK APPROACH ; CURRENT DENSITIES ; FINITE NUCLEI ; EXOTIC NUCLEI ; MOMENTS ; DISTRIBUTIONS ; RADIUS ; HALOS ; ORBIT |
| Indexed By | SCI |
| Language | 英语 |
| WOS Research Area | Physics |
| WOS Subject | Physics, Nuclear |
| WOS ID | WOS:000357858700003 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://libir.pmo.ac.cn/handle/332002/14797 |
| Collection | 暗物质和空间天文实验室 |
| Affiliation | 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 |
| Recommended Citation 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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| 2015034.pdf（379KB） | 开放获取 | Apache License | View Application Full Text | |||
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