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===Joel's Check of Dominic's Logic and Numbers=== Let's plug in values of the physical units that we have tabulated in a [[Appendix/VariablesTemplates|Variables Appendix]] to see if we agree with Dominic's conversions. <table border="0" align="center" cellpadding="8"> <tr> <td align="right"> <math> \frac{c^2}{\Re} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{(3\times 10^{10})^2}{8.314\times 10^7}~\mathrm{cgs} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 1.083\times 10^{13}~\mathrm{K} </math> </td> </tr> <tr> <td align="right"> <math> \biggl(\frac{\Re^4}{c^4 G a_\mathrm{rad}}\biggr)^{1/2} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{(8.314\times 10^7)^2}{(3\times 10^{10})^2 (6.674\times 10^{-8})^{1/2}(7.566\times 10^{-15})^{1/2}}~\mathrm{cgs} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 3.418\times 10^{5}~\mathrm{cm} </math> </td> </tr> <tr> <td align="right"> <math> \biggl(\frac{\Re^4}{c^6 G a_\mathrm{rad}}\biggr)^{1/2} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{(8.314\times 10^7)^2}{(3\times 10^{10})^3 (6.674\times 10^{-8})^{1/2}(7.566\times 10^{-15})^{1/2}}~\mathrm{cgs} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 1.139\times 10^{-5}~\mathrm{s} </math> </td> </tr> <tr> <td align="right"> <math> \biggl(\frac{\Re^4}{G^3 a_\mathrm{rad}}\biggr)^{1/2} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{(8.314\times 10^7)^2}{(6.674\times 10^{-8})^{3/2}(7.566\times 10^{-15})^{1/2}}~\mathrm{cgs} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 4.609\times 10^{33}~\mathrm{g} </math> </td> </tr> </table> Hence, <table border="1" align="center" cellpadding="8"> <tr> <td colspan="3" align="center"> <font color="blue"><b>General Relations</b></font> </td> </tr> <tr> <td align="right"> <math> \frac{T_\mathrm{cgs}}{T_\mathrm{code}} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 1.083\times 10^{13}~\mathrm{K} \biggl( \frac{\tilde{r}}{\tilde{c}^2} \biggr) </math> </td> </tr> <tr> <td align="right"> <math> \frac{\ell_\mathrm{cgs}}{\ell_\mathrm{code}} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 3.418\times 10^{5}~\mathrm{cm} \biggl( \frac{\tilde{c}^4 \tilde{g} \tilde{a} }{\tilde{r}^4} \biggr)^{1/2} </math> </td> </tr> <tr> <td align="right"> <math> \frac{t_\mathrm{cgs}}{t_\mathrm{code}} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 1.139\times 10^{-5}~\mathrm{s} \biggl( \frac{\tilde{c}^6 \tilde{g} \tilde{a} }{\tilde{r}^4} \biggr)^{1/2} </math> </td> </tr> <tr> <td align="right"> <math> \frac{m_\mathrm{cgs}}{m_\mathrm{code}} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 4.609\times 10^{33}~\mathrm{g} \biggl( \frac{\tilde{g}^3 \tilde{a} }{\tilde{r}^4} \biggr)^{1/2} </math> </td> </tr> </table> For the '''Case A''' parameter values adopted by Dominic, above, and for the particular SCF-code-generated model provided by Wes, I derive, <table border="1" align="center" cellpadding="8"> <tr> <td colspan="5" align="center"> <b>Case A</b> </td> </tr> <tr> <td align="right"> <math> R_\mathrm{Accretor} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 3.418\times 10^{5}~\mathrm{cm} \biggl[ \frac{198^4 \times 0.044 }{(0.44)^4 } \biggr]^{1/2} \times 0.40 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 5.8\times 10^{9}~\mathrm{cm} = 0.083~\mathrm{R}_\odot </math> </td> </tr> <tr> <td align="right"> <math> P_\mathrm{orbit} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 1.139\times 10^{-5}~\mathrm{s} \biggl[ \frac{198^6 \times 0.044 }{(0.44)^4} \biggr]^{1/2} \times 31 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 2.97\times 10^{3}~\mathrm{s} = 49.5 ~\mathrm{minutes} </math> </td> </tr> <tr> <td align="right"> <math> M_\mathrm{total} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 4.609\times 10^{33}~\mathrm{g} \biggl[ \frac{0.044 }{(0.44)^4 } \biggr]^{1/2} \times 0.85 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 4.245\times 10^{33}~\mathrm{g} = 2.1~\mathrm{M}_\odot </math> </td> </tr> </table> These values do not agree with the ones derived by Dominic. <table border="1" width="75%" cellpadding="8" align="center"> <tr> <td align="center"> <font color="red">Possible Point of Confusion/Disagreement</font> </td> </tr> <tr><td align="left"> NOTE: Either Dominic wrote the wrong values on my whiteboard or I copied them down incorrectly, but based on the [http://www.phys.lsu.edu/~tohline/clayton/q07.pdf SCF-code parameters] that were given to me by Wes Even, in dimensionless code units the model parameters should be: <math>[M_\mathrm{total}]_\mathrm{code} = 0.0237</math> and <math>[R_\mathrm{Accretor}]_\mathrm{code} = 0.273</math> and <math>[P_\mathrm{orbit}]_\mathrm{code} = 31.19</math>; the orbital ''separation'' is <math>[a_\mathrm{separation}]_\mathrm{code} = 0.83938</math>. Combining ''these'' values with Dominic's '''Case A''' parameter values gives: * <math>[M_\mathrm{total}]_\mathrm{cgs} = 0.059 M_\odot</math>; * <math>[R_\mathrm{Accretor}]_\mathrm{cgs} = 0.057 R_\odot</math>; * <math>[P_\mathrm{orbit}]_\mathrm{cgs} = 50~\mathrm{minutes}</math>; and * <math>[a_\mathrm{separation}]_\mathrm{cgs} = 0.174 R_\odot</math>. </td></tr> <tr> <td align="left"> On 7/24/2010, Joel checked this boxed-in group of numbers against a "polytropic unit conversion spreadsheet" that he developed while at the Lorentz Institute in the Fall of 2010. They are all consistent with Wes Even's SCF-generated Q07 model. </td> </tr> </table>
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