The Dipole Magnetic Field and Spin-down Evolutions of the High Braking Index Pulsar PSR J1640-4631
文献类型:期刊论文
作者 | Wang, Na2,3; Wang, Wei5,6; Gao, Zhi-Fu2,3; Shan, Hao2; Li, Xiang-Dong1,4 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2017-11-01 |
卷号 | 849期号:1页码:19 |
ISSN号 | 0004-637X |
关键词 | Ism: Supernova Remnants Magnetic Field: Neutron Pulsars: Individual (J1640-4631) Stars: Evolution |
DOI | 10.3847/1538-4357/aa8f49 |
产权排序 | 1 |
文献子类 | Article |
英文摘要 | In this work, we interpreted the high braking index of PSR J1640-4631 with a combination of the magnetodipole radiation and dipole magnetic field decay models. By introducing a mean rotation energy conversion coefficient (zeta) over bar, the ratio of the total high-energy photon energy to the total rotation energy loss in the whole life of the pulsar, and combining the pulsar's high-energy and timing observations with a reliable nuclear equation of state, we estimate the pulsar's initial spin period, P-0 similar to (17-44) ms, corresponding to the moment of inertia I similar to (0.8-2.1) x 10(45) g cm(2). Assuming that PSR J1640-4631 has experienced a long-term exponential decay of the dipole magnetic field, we calculate the true age t(age), the effective magnetic field decay timescale tau(D), and ;the initial surface dipole magnetic field at the pole B-p (0) of the pulsar to be 2900-3100 yr, 1.07(2) x 10(5) yr, and (1.84-4.20) x 10(13) G, respectively. The measured braking index of n = 3.15(3) for PSR J1640-4631 is attributed to its long-term dipole magnetic field decay and a low magnetic field decay rate, dB(p)/dt similar to -(1.66-3.85) x 10(8) G yr(-1). Our model can be applied to both the high braking index (n > 3) and low braking index (n < 3) pulsars, tested by the future polarization, timing, and high-energy observations of PSR J1640-4631. |
URL标识 | 查看原文 |
WOS关键词 | Isolated Neutron-stars ; Gamma-ray Repeaters ; Equation-of-state ; Single Radio Pulsars ; Supernova-remnants ; Magnetothermal Evolution ; Population Synthesis ; Young Pulsar ; High-energy ; Decay |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000425465900001 |
资助机构 | National Basic Research Program of China grants 973 Programs(2015CB857100) ; West Light Foundation of CAS(XBBS-2014-23, XBBS-2014-22, 2172201302) ; Chinese National Science Foundation(11673056, 11622326, 11273051, 11373006, 11133004, 11173042) ; CAS(XDB23000000) ; National Program on Key Research and Development Project(2016YFA0400803) |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/1897] |
专题 | 脉冲星研究团组 新疆天文台_计算机技术室 新疆天文台_110米口径全可动射电望远镜(SmART)_110米大口径全可动射电望远镜关键技术研究(973项目)_课题1:大样本射电天体的观测和前沿问题研究 |
通讯作者 | Gao, Zhi-Fu |
作者单位 | 1.Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210046, Jiangsu, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China 4.Nanjing Univ, Dept Astron, Nanjing 210046, Jiangsu, Peoples R China 5.Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China 6.Chiese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, Na,Wang, Wei,Gao, Zhi-Fu,et al. The Dipole Magnetic Field and Spin-down Evolutions of the High Braking Index Pulsar PSR J1640-4631[J]. ASTROPHYSICAL JOURNAL,2017,849(1):19. |
APA | Wang, Na,Wang, Wei,Gao, Zhi-Fu,Shan, Hao,&Li, Xiang-Dong.(2017).The Dipole Magnetic Field and Spin-down Evolutions of the High Braking Index Pulsar PSR J1640-4631.ASTROPHYSICAL JOURNAL,849(1),19. |
MLA | Wang, Na,et al."The Dipole Magnetic Field and Spin-down Evolutions of the High Braking Index Pulsar PSR J1640-4631".ASTROPHYSICAL JOURNAL 849.1(2017):19. |
入库方式: OAI收割
来源:新疆天文台
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