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Volumn 104, Issue 2, 2000, Pages 325-358

Axisymmetric simulations of rotating Stellar collapse in full general relativity: Criteria for prompt collapse to black holes

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EID: 0034346050     PISSN: 0033068X     EISSN: None     Source Type: Journal    
DOI: 10.1143/PTP.104.325     Document Type: Article
Times cited : (81)

References (46)
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    • But, for a special class of gauge conditions with appropriate prescriptions, it is still possible to preserve the accuracy and stability without artificial viscosity (e.g., D. Garfinkle, personal communication)
    • But, for a special class of gauge conditions with appropriate prescriptions, it is still possible to preserve the accuracy and stability without artificial viscosity (e.g., D. Garfinkle, personal communication).
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    • note
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    • -1/2 is smaller than 3.6, a black hole could be formed for the case in which the gravitational binding energy is sufficiently large initially. Hence, the value 3.6 is not an absolute threshold, even for q = 0, although it could be a good guideline
    • -1/2 is smaller than 3.6, a black hole could be formed for the case in which the gravitational binding energy is sufficiently large initially. Hence, the value 3.6 is not an absolute threshold, even for q = 0, although it could be a good guideline.
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    • We reached this conclusion because convergence was not well achieved when Ν was increased
    • We reached this conclusion because convergence was not well achieved when Ν was increased.
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    • max denotes the maximum density at t = 0
    • max denotes the maximum density at t = 0.
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    • g, could maintain a stable orbit
    • g, could maintain a stable orbit.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.