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Formlaghys BSSN

Veih Wikipedia.

She formlaghys y chonastaght chadjin eh formlaghys BSSN (formlaghys Baumgarte, Shapiro, Shibata, Nakamura). V'eh er ny lhiasaghey lesh Thomas W. Baumgarte, Stuart L. Shapiro, Masaru Shibata, as Takashi Nakamura eddyr ny bleeantyn 1987 as 1999.[1] She caghlaa lesh formlaghys ADM t'eh, v'er ny lhiasaghey ayns ny 1950yn.

She formlaghys Hamilton nagh vel lowal yn-soyllaghyn earrooagh shickyr as foddey-çhiarrymagh. 'Syn ormlaghys BSSN, ta cormidyn ADM er nyn gaghlaa lesh cur stiagh ceaghlee choonee. Ta'n formlaghys er ny ve prowit son aafilley foddey-çhiarrymagh dy honnyn ym-hayrnagh linnagh as er ny ve ymmydit son cooishyn eigsoylagh lheid as yn-soylley yn aafilley neu-linnagh tonnyn ym-hayrnagh ny aafilley as covuilley [[towl doo|tuill ghoo.[2][3]

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  1. Jinho Kim (2008-07-28). "General Relativistic Hydrodynamics Using BSSN formalism" (PDF). Ollooscoill Ashoonagh Seoul. Er ny hashtey veih yn lhieggan bunneydagh (PDF) er 2012-03-27. Feddynit magh er 2009-10-19.
  2. Masaru Shibata (Jerrey Fouyir 2004). "Status of numerical relativity". Academee Sheansyn yn Injey. Feddynit magh er 2009-10-19.
  3. Takashi Nakamura (2006). "Formation of black hole and emission of gravitational waves". Proceedings of the Japan Academy, Series B. Ym-lioar 82 (9): 311–327. doi:10.2183/pjab.82.311. PMID 25792793. Bibcode2006PJAB...82..311N.