Improved fast-rotating black hole evolution simulations with modified Baumgarte-Shapiro-Shibata-Nakamura formulation
文献类型:期刊论文
作者 | Yo, Hwei-Jang1; Cao, Zhoujian2,3![]() |
刊名 | PHYSICAL REVIEW D
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出版日期 | 2015-07-21 |
卷号 | 92期号:2页码:10 |
ISSN号 | 1550-7998 |
DOI | 10.1103/PhysRevD.92.024034 |
英文摘要 | Different formulations of Einstein's equations used in numerical relativity can affect not only the stability but also the accuracy of numerical simulations. In the original Baumgarte-Shapiro-Shibata-Nakamura (BSSN) formulation, the loss of the angular momentum, J, is non-negligible in highly spinning single black hole evolutions. This loss also appears, usually right after the merger, in highly spinning binary black hole simulations, The loss of J may be attributed to some unclear numerical dissipation. Reducing unphysical dissipation is expected to result in more stable and accurate evolutions. In the previous work [H.-J. Yo et al., Phys. Rev. D 86, 064027 (2012).] we proposed several modifications which are able to prevent black hole evolutions from the unphysical dissipation, and the resulting simulations are more stable than in the traditional BSSN formulation. Specifically, these three modifications (M1, M2, and M3) enhance the effects of stability, hyperbolicity, and dissipation of the formulation. We experiment further in this work with these modifications, and demonstrate that these modifications improve the accuracy and also effectively suppress the loss of J, particularly in the black hole simulations with an initially large ratio of J and a square of the ADM mass. |
资助项目 | National Science Council[NSC102-2112-M-006-014-MY2] ; Headquarters of University Advancement at the National Cheng Kung University - Ministry of Education, Taiwan, Republic of China ; NSFC[11375260] |
WOS研究方向 | Astronomy & Astrophysics ; Physics |
语种 | 英语 |
WOS记录号 | WOS:000358257600002 |
出版者 | AMER PHYSICAL SOC |
源URL | [http://ir.amss.ac.cn/handle/2S8OKBNM/20398] ![]() |
专题 | 应用数学研究所 |
通讯作者 | Yo, Hwei-Jang |
作者单位 | 1.Natl Cheng Kung Univ, Dept Phys, Tainan 701, Taiwan 2.Chinese Acad Sci, Acad Math & Syst Sci, Inst Appl Math, Beijing 100190, Peoples R China 3.Chinese Acad Sci, Acad Math & Syst Sci, LSEC, Beijing 100190, Peoples R China 4.Natl Ctr High Performance Comp, Hsinchu 300, Taiwan |
推荐引用方式 GB/T 7714 | Yo, Hwei-Jang,Cao, Zhoujian,Lin, Chun-Yu,et al. Improved fast-rotating black hole evolution simulations with modified Baumgarte-Shapiro-Shibata-Nakamura formulation[J]. PHYSICAL REVIEW D,2015,92(2):10. |
APA | Yo, Hwei-Jang,Cao, Zhoujian,Lin, Chun-Yu,&Pan, Hsing-Po.(2015).Improved fast-rotating black hole evolution simulations with modified Baumgarte-Shapiro-Shibata-Nakamura formulation.PHYSICAL REVIEW D,92(2),10. |
MLA | Yo, Hwei-Jang,et al."Improved fast-rotating black hole evolution simulations with modified Baumgarte-Shapiro-Shibata-Nakamura formulation".PHYSICAL REVIEW D 92.2(2015):10. |
入库方式: OAI收割
来源:数学与系统科学研究院
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