2012年9月
Three-dimensional evolution of differentially rotating magnetized neutron stars
Physical Review D
- ,
- ,
- 巻
- 86
- 号
- 6
- 開始ページ
- 064008
- 終了ページ
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1103/PhysRevD.86.064008
- 出版者・発行元
- AMER PHYSICAL SOC
We construct a new three-dimensional general relativistic magnetohydrodynamics code, in which a fixed mesh refinement technique is implemented. To ensure the divergence-free condition as well as the magnetic flux conservation, we employ the method by Balsara [J. Comp. Physiol. 174, 614 (2001); J. Comp. Phys. 228, 5040 (2009)]. Using this new code, we evolve differentially rotating magnetized neutron stars, and find that a magnetically driven outflow is launched from the star exhibiting a kink instability. The matter ejection rate and Poynting flux are still consistent with our previous finding [M. Shibata, Y. Suwa, K. Kiuchi, and K. Ioka, Astrophys. J. 734, L36 (2011)] obtained in axisymmetric simulations.
- リンク情報
- ID情報
-
- DOI : 10.1103/PhysRevD.86.064008
- ISSN : 2470-0010
- eISSN : 2470-0029
- ORCIDのPut Code : 51254209
- Web of Science ID : WOS:000308292300007