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Volumn 437, Issue 1, 2013, Pages

Beyond second-order convergence in simulations of binary neutron stars in full general relativity

Author keywords

Gravitational waves stars; Neutron

Indexed keywords


EID: 84890040304     PISSN: 17453925     EISSN: 17453933     Source Type: Journal    
DOI: 10.1093/mnrasl/slt137     Document Type: Article
Times cited : (236)

References (40)
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    • preprint (arXiv:1307.5307)
    • Hinder I. et al., 2013, preprint (arXiv:1307.5307)
    • (2013)
    • Hinder, I.1
  • 25
    • 84890081841 scopus 로고    scopus 로고
    • preprint (arXiv:1304.6077)
    • Mroue A. H. et al., 2013, preprint (arXiv:1304.6077)
    • (2013)
    • Mroue, A.H.1
  • 29
  • 35
    • 84890110263 scopus 로고    scopus 로고
    • Lecture Notes on ICASE Report 97-65 (NASA CR- 97-206253), Essentially Non-Oscillatory and Weighted Essentially Non-Oscillatory Schemes for Hyperbolic Conservation Laws. NASA Langley Research Center, available at:
    • Shu C. W., 1997, Lecture Notes on ICASE Report 97-65 (NASA CR- 97-206253), Essentially Non-Oscillatory and Weighted Essentially Non-Oscillatory Schemes for Hyperbolic Conservation Laws. NASA Langley Research Center, available at: http://ntrs.nasa.gov/archive/ nasa/casi.ntrs.nasa.gov/19980007543_1998045663.pdf)
    • (1997)
    • Shu, C.W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.