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===Scale Factor Expressions=== We are now in a position to express the two key scale factors purely in terms of the two key T3 coordinates. First, we note that, <div align="center"> <math> \ell^{2} = [\varpi^2 + 4z^2]^{-1} = \frac{2}{\lambda_2^2(\Lambda - 1)\Lambda} , </math> </div> and, <div align="center"> <math> \biggl(\frac{\lambda_1}{\lambda_2}\biggr)^2 = \frac{1}{4}\Chi^2 = \frac{1}{4}(\Lambda^2 -1) = \frac{1}{4}(\Lambda -1)(\Lambda +1) . </math> </div> Hence, <table border="0" align="center" cellpadding="5"> <tr> <td align="right"> <math> h_1^2 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \lambda_1^2 \ell^2 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{1}{2}\biggl[ \frac{\Lambda + 1}{\Lambda} \biggr] ; </math> </td> </tr> <tr> <td align="right"> <math> h_2^2 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> (q^2-1)\biggl( \frac{\varpi z \ell}{\lambda_2} \biggr)^2 </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{1}{8}~ \frac{(\Lambda - 1)^2}{\Lambda} . </math> </td> </tr> </table> We note also that, <table border="0" align="center" cellpadding="5"> <tr> <td align="right"> <math> \frac{d\Lambda}{dt} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{d}{dt}\biggl[ 1+(2\lambda_1/\lambda_2)^2 \biggr]^{1/2} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \biggl[ \frac{\Lambda^2-1}{\Lambda} \biggr] \frac{d\ln(\lambda_1/\lambda_2)}{dt} . </math> </td> </tr> </table> Hence, starting from the [[Appendix/Ramblings/T3Integrals#Logarithmic_Derivatives_of_Scale_Factors|''general'' expression for <math>d\ln h_2/dt</math> derived elsewhere]], we deduce that, <table border="0" align="center" cellpadding="5"> <tr> <td align="right"> <math> \frac{d\ln h_2}{dt} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> 2 h_1^4\frac{d}{dt}\biggl[ \ln(\lambda_1/\lambda_2) \biggr] </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{1}{2} \biggl( \frac{\Lambda +1}{\Lambda} \biggr)^2 \biggl[ \frac{\Lambda^2-1}{\Lambda} \biggr]^{-1} \frac{d\Lambda}{dt} </math> </td> <td align="center"> <math> = </math> </td> <td align="left"> <math> \frac{1}{2} \biggl( \frac{\Lambda +1}{\Lambda-1} \biggr) \frac{d\ln\Lambda}{dt} . </math> </td> </tr> </table> (This identical expression also can be derived straightforwardly from the ''specific'' expression for <math>h_2</math> given above.) From the expression given above for <math>h_1</math>, we also deduce that, <div align="center"> <math> \frac{d\ln h_1}{dt} = - \frac{1}{2(\Lambda + 1)} \frac{d\ln\Lambda}{dt} . </math> </div> As a check, we note that the relationship between <math>d\ln h_1/dt</math> and <math>d\ln h_2/dt</math> in this ''specific'' case (<i>i.e.</i>, <math>q^2 = 2</math>) matches the ''general'' relationship between these two logarithmic time-derivatives that has been [[Appendix/Ramblings/T3Integrals#Logarithmic_Derivatives_of_Scale_Factors|derived elsewhere]], namely, <div align="center"> <math> (h_1 \lambda_1)^2 \frac{d\ln h_1}{dt} + (h_2 \lambda_2)^2 \frac{d\ln h_2}{dt} = 0 . </math> </div>
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