Appendix/Ramblings/BdHN: Difference between revisions
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=Binary-driven | =Binary-driven Hypernovae= | ||
The material presented here builds on our separate discussion of [[Appendix/Ramblings/TurningPoints#Close_Binary_Stars|close binary stars]]. | The material presented here builds on our separate discussion of [[Appendix/Ramblings/TurningPoints#Close_Binary_Stars|close binary stars]]. | ||
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==Setup== | ==Setup== | ||
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=Critique= | =Critique= | ||
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C. See, for example, the expression for L_1 immediately following Eq. (1) on p. 165 of Darwin, G. H. (1906, Philosophical Transactions of the Royal Society A, Vol. 206, 161). | C. See, for example, the expression for L_1 immediately following Eq. (1) on p. 165 of Darwin, G. H. (1906, Philosophical Transactions of the Royal Society A, Vol. 206, 161). | ||
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==Other== | |||
===Trial Pieces=== | |||
As a case in point, their toy model "before fission" is a (10 solar-mass) Maclaurin spheroid; next, they envision that fission occurs when the initial CO_star is rotating sufficiently fast that its eccentricity places it at the point along the Maclaurin sequence where the Jacobi sequence bifurcates (e = 0.8127); finally, their toy model "after fission" is a (1.5 solar-mass) Jacobi ellipsoid paired with an 8.5 solar-mass Maclaurin spheroid; . This is inaccurate depiction of the classical fission theory [see note 1, below]. | As a case in point, their toy model "before fission" is a (10 solar-mass) Maclaurin spheroid; next, they envision that fission occurs when the initial CO_star is rotating sufficiently fast that its eccentricity places it at the point along the Maclaurin sequence where the Jacobi sequence bifurcates (e = 0.8127); finally, their toy model "after fission" is a (1.5 solar-mass) Jacobi ellipsoid paired with an 8.5 solar-mass Maclaurin spheroid; . This is inaccurate depiction of the classical fission theory [see note 1, below]. | ||
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<li>Ill-advised to refer to the ''new'' NS as "νNS" because, in this context, readers might reasonably associate the greek letter, ν, with neutrinos. </li> | <li>Ill-advised to refer to the ''new'' NS as "νNS" because, in this context, readers might reasonably associate the greek letter, ν, with neutrinos. </li> | ||
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=See Also= | =See Also= | ||
Latest revision as of 12:59, 4 July 2023
Binary-driven Hypernovae
The material presented here builds on our separate discussion of close binary stars.
HIDDEN as of 4 July 2023.
See Also
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |