2010 Fiscal Year Final Research Report
Quasi-equilibriums of magnetized binary neutron stars and initial data for numerical relativity simulations
Project/Area Number |
20540275
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Research Category |
Grant-in-Aid for Scientific Research (C)
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Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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Research Institution | University of the Ryukyus |
Principal Investigator |
URYU Koji University of the Ryukyus, 理学部, 准教授 (40457693)
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Research Collaborator |
GOURGOULHON Eric CNRS/Observatoire de Paris・Universite Paris Diderot, Directeur de recherche
MARKAKIS Charalampos University of Wisconsin-Milwaukee, 大学院生(博士課程)
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Project Period (FY) |
2008 – 2010
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Keywords | 相対論・重力(理論) / 重力波 / 相対論的宇宙物理学 / 数値相対論 / 連星中性子星 / 高速回転星 / ブラックホール-中性子星連星 / 中性子星磁場 |
Research Abstract |
Formulations for computing quasi-equilibrium of magnetized binary neutron stars and their generalized thermodynamic laws are derived. We develop a new code, Cocal-Compact Object CALculator, to calculate structures of compact objects in quasi-equilibriums, and successfully compute, for example, triaxially deformed rapidly rotating neutron stars. Quasi-equilibrium solutions for binary neutron stars are also calculated, and they are provided as initial data sets for simulations of binary inspirals. Gravitational waveforms obtained the simulations are analyzed.
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Research Products
(10 results)
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[Presentation] Magnetized binary compact objects2010
Author(s)
Eric Gourgoulhon, Koji Uryu, Charalampos Markakis
Organizer
19^<th> International Conference on General Relativity and Gravitation (GR19)
Place of Presentation
Mexico City, Mexico
Year and Date
20100705-20100709
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