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Volumn 89, Issue 6, 2014, Pages

Accretion disks around binary black holes of unequal mass: General relativistic magnetohydrodynamic simulations near decoupling

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EID: 84898714624     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.89.064060     Document Type: Article
Times cited : (159)

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    • Condition (III) is satisfied everywhere shortly after our evolutions begin because magnetic winding converts the poloidal magnetic field into toroidal, thereby decreasing (Equation presented). Our high-resolution grids satisfy condition (II) in the innermost parts of the disk even after the evolution begins.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.