Dynamic collapses of relativistic degenerate stellar cores and radiation pressure dominated stellar interiors
文献类型:期刊论文
作者 | Shi, Chun-Hui1,2,3,5; Lou, Yu-Qing2,3,4 |
刊名 | NEW ASTRONOMY |
出版日期 | 2018-04-01 |
卷号 | 60页码:14-21 |
ISSN号 | 1384-1076 |
关键词 | Black hole physics Dense matter Hydrodynamics Stars: Neutron Stars: population III Supernovae: general |
DOI | 10.1016/j.newast.2017.07.010 |
英文摘要 | We investigate and explore self-similar dynamic radial collapses of relativistic degenerate stellar cores (RDSCs) and radiation pressure dominated stellar interiors (RPDSIs) of spherical symmetry by invoking a conventional polytropic (CP) equation of state (EoS) with a constant polytropic index gamma = 4/3 and by allowing free-fall non-zero RDSC or RPDSI surface mass density and pressure due to their sustained physical contact with the outer surrounding stellar envelopes also in contraction. Irrespective of the physical triggering mechanisms (including, e.g., photodissociation, electron-positron pair instability, general relativistic instability etc.) for initiating such a self-similar dynamically collapsing RDSC or RPDSI embedded within a massive star, a very massive star (VMS) or a supermassive star (SMS) in contraction and by comparing with the Schwarzschild radii associated with their corresponding RDSC/RPDSI masses, the emergence of central black holes in a wide mass range appears inevitable during such RDSC/RPDSI dynamic collapses inside massive stars, VMSs, and SMSs, respectively. Radial pulsations of progenitor cores or during a stellar core collapse may well leave imprints onto collapsing RDSCs/RPDSIs towards their self-similar dynamic evolution. Massive neutron stars may form during dynamic collapses of RDSC inside massive stars in contraction under proper conditions. (C) 2017 Elsevier B.V. All rights reserved. |
WOS关键词 | APPROACHING SCHWARZSCHILD LIMIT ; SELF-SIMILAR DYNAMICS ; MASSIVE STARS ; GENERAL-RELATIVITY ; SUPERMASSIVE STARS ; BLACK-HOLES ; INSTABILITY ; SUPERNOVAE ; EVOLUTION ; EXPLOSION |
资助项目 | Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research[2012CB821800] ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research[2012CB821802] ; National Natural Science Foundation of China (NSFC) at Tsinghua University[10373009] ; National Natural Science Foundation of China (NSFC) at Tsinghua University[10533020] ; National Natural Science Foundation of China (NSFC) at Tsinghua University[11073014] ; National Natural Science Foundation of China (NSFC) at Tsinghua University[11473018] ; National Natural Science Foundation of China (NSFC) at Tsinghua University[11773019] ; MOST[2014YQ030975] ; Tsinghua Centre for Astrophysics ; Tsinghua University Initiative Scientific Research Programme[20111081008] ; Special Research Fund for Doctoral Programme[20050003088] ; Special Research Fund for Doctoral Programme[200800030071] ; Special Research Fund for Doctoral Programme[20110002110008] ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS)[XDB23000000] ; CAS ; 985 grants ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | ELSEVIER SCIENCE BV |
WOS记录号 | WOS:000417773200003 |
资助机构 | Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; MOST ; MOST ; Tsinghua Centre for Astrophysics ; Tsinghua Centre for Astrophysics ; Tsinghua University Initiative Scientific Research Programme ; Tsinghua University Initiative Scientific Research Programme ; Special Research Fund for Doctoral Programme ; Special Research Fund for Doctoral Programme ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; CAS ; CAS ; 985 grants ; 985 grants ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; MOST ; MOST ; Tsinghua Centre for Astrophysics ; Tsinghua Centre for Astrophysics ; Tsinghua University Initiative Scientific Research Programme ; Tsinghua University Initiative Scientific Research Programme ; Special Research Fund for Doctoral Programme ; Special Research Fund for Doctoral Programme ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; CAS ; CAS ; 985 grants ; 985 grants ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; MOST ; MOST ; Tsinghua Centre for Astrophysics ; Tsinghua Centre for Astrophysics ; Tsinghua University Initiative Scientific Research Programme ; Tsinghua University Initiative Scientific Research Programme ; Special Research Fund for Doctoral Programme ; Special Research Fund for Doctoral Programme ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; CAS ; CAS ; 985 grants ; 985 grants ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; Ministry of Science and Technology (MOST) under the State Key Development Programme for Basic Research ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; National Natural Science Foundation of China (NSFC) at Tsinghua University ; MOST ; MOST ; Tsinghua Centre for Astrophysics ; Tsinghua Centre for Astrophysics ; Tsinghua University Initiative Scientific Research Programme ; Tsinghua University Initiative Scientific Research Programme ; Special Research Fund for Doctoral Programme ; Special Research Fund for Doctoral Programme ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Programme of the Chinese Academy of Sciences (CAS) ; CAS ; CAS ; 985 grants ; 985 grants ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Yangtze Endowment from the Ministry of Education (MoE) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University ; Advanced Micro Devices (AMD) scholarship at Tsinghua University |
源URL | [http://ir.bao.ac.cn/handle/114a11/37329] |
专题 | 中国科学院国家天文台 |
通讯作者 | Lou, Yu-Qing |
作者单位 | 1.Chinese Acad Sci, China Chile Joint Ctr Astron, South Amer Ctr Astron, Camino El Observ 1515, Santiago, Chile 2.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 3.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China 4.Tsinghua Univ, Tsinghua Natl Astron Observ China NAOC Joint Res, Beijing 100084, Peoples R China 5.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Shi, Chun-Hui,Lou, Yu-Qing. Dynamic collapses of relativistic degenerate stellar cores and radiation pressure dominated stellar interiors[J]. NEW ASTRONOMY,2018,60:14-21. |
APA | Shi, Chun-Hui,&Lou, Yu-Qing.(2018).Dynamic collapses of relativistic degenerate stellar cores and radiation pressure dominated stellar interiors.NEW ASTRONOMY,60,14-21. |
MLA | Shi, Chun-Hui,et al."Dynamic collapses of relativistic degenerate stellar cores and radiation pressure dominated stellar interiors".NEW ASTRONOMY 60(2018):14-21. |
入库方式: OAI收割
来源:国家天文台
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