Editing
Appendix/Mathematics/ToroidalConfusion
(section)
Jump to navigation
Jump to search
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=Cohl's Response to My (May 2018) Email Query= ==Proper Interpretation of DLMF Expression== Most of the confusion expressed above stems from the DLMF's use of '''bold''' fonts, such as the function on the left-hand side of expression #3, above — that is, the Whipple formula from [https://dlmf.nist.gov/14.19.v §14.19 of DLMF], <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\boldsymbol{Q}^{m}_{n-\frac{1}{2}}\left(\cosh\xi\right)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\Gamma\left(m-n+ \tfrac{1}{2}\right)}{\Gamma\left(m+n+\tfrac{1}{2}\right)}\left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) \, . </math> </td> </tr> </table> What has been missing in my discussion is an appreciation of the following relationship between [http://dlmf.nist.gov/14.3.E10 '''bold''' and plain-text function names], <div align="center"> <math> \boldsymbol{Q}^{\mu}_{\nu}\left(x\right)=e^{-\mu\pi i}\frac{Q^{\mu}_{\nu}\left(x\right)}{\Gamma\left(\nu+\mu+1\right)}. </math> </div> After making the substitutions, <math>~\mu \rightarrow m</math> and <math>~\nu \rightarrow (n-\tfrac{1}{2})</math>, the Whipple formula displayed above as expression #3 becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~e^{-m\pi i}\frac{Q^{m}_{n-\frac{1}{2}}\left(\cosh\xi\right)}{\Gamma\left(n+m+\tfrac{1}{2}\right)}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\Gamma\left(m-n+ \tfrac{1}{2}\right)}{\Gamma\left(m+n+\tfrac{1}{2}\right)}\left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ Q^{m}_{n-\frac{1}{2}}\left(\cosh\xi\right)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~e^{m\pi i} \Gamma\left(m-n+\tfrac{1}{2}\right)\left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(-1)^m \Gamma\left(m-n+\tfrac{1}{2}\right)\left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) \, , </math> </td> </tr> </table> which matches expression #2, above. But it does not ''appear'' to match expressions #1 or #4. <table border="1" cellpadding="5" align="center" width="80%"><tr><td align="left"> The standard "Euler reflection formula for gamma functions" is usually presented in the form, {{ Math/EQ_Gamma01 }} If we make the association, <div align="center"> <math>~z \leftrightarrow (m - n + \tfrac{1}{2}) \, ,</math> </div> with <math>~m</math> and <math>~n</math> both being either zero or a positive integer, then, this Euler reflection formula becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\Gamma(m - n + \tfrac{1}{2}) ~ \Gamma(n - m + \tfrac{1}{2} )</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\pi \biggl\{ \sin\biggl[ \pi(m - n + \tfrac{1}{2}) \biggr] \biggr\}^{-1}</math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\pi (-1)^{m+n} \, .</math> </td> </tr> </table> </td></tr></table> However, in our situation the so-called "Euler reflection formula for gamma functions" gives the relation, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{\pi (-1)^{m+n}}{\Gamma(n-m+\frac{1}{2}) }</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\Gamma(m-n+\tfrac{1}{2}) \, .</math> </td> </tr> </table> </div> Hence, we may also write, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ Q^{m}_{n-\frac{1}{2}}\left(\cosh\xi\right)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(-1)^m \biggl[ \frac{\pi (-1)^{m+n}}{\Gamma(n-m+\frac{1}{2}) } \biggr] \left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{(-1)^n \pi }{\Gamma(n-m+\frac{1}{2}) } \left(\frac{\pi}{2 \sinh\xi}\right)^{1 / 2}P^{n}_{m-\frac{1}{2}}\left(\coth\xi\right) \, , </math> </td> </tr> </table> which matches expressions #1 and #4. So everything appears to be in agreement! Hooray! ==Derivation From Scratch== Whenever he deals with these types of relations, Cohl usually begins with, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr><th align="center" colspan="3"><font color="maroon">Expression #5</font></th></tr> <tr> <td align="right"> <math>~Q^\mu_\nu(\cosh\eta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \sqrt{\frac{\pi}{2}} ~\Gamma(\nu + \mu + 1) ~e^{i\mu\pi} \biggl[ \frac{1}{\sinh^2\eta} \biggr]^{1 / 4} P^{-\nu-\frac{1}{2}}_{-\mu - \frac{1}{2}} (\coth\eta) </math> </td> </tr> </table> </div> Making the pair of substitutions, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\nu</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~n - \frac{1}{2} \, ,</math> </td> <td align="center"> </td> <td align="right"> <math>~n ~~\in</math> </td> <td align="left"> <math>~\mathbb{N}_0 = \{ 0, 1, 2, \cdots\} \, ,</math> </td> </tr> <tr> <td align="right"> <math>~\mu</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~m \, ,</math> </td> <td align="center"> </td> <td align="right"> <math>~m ~~\in</math> </td> <td align="left"> <math>~\mathbb{N}_0 = \{ 0, 1, 2, \cdots\} \, ,</math> </td> </tr> </table> </div> we also have, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\nu + \mu +1</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~n - \frac{1}{2} + m + 1</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~n + m + \frac{1}{2} \, ,</math> </td> </tr> <tr> <td align="right"> <math>~-\mu - \frac{1}{2}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~-m-\frac{1}{2} \, ,</math> </td> <td align="center"> </td> <td align="left"> </td> </tr> <tr> <td align="right"> <math>~-\nu - \frac{1}{2}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~-\biggl(n - \frac{1}{2}\biggr)-\frac{1}{2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~-n \, , </math> </td> </tr> <tr> <td align="right"> <math>~e^{i\mu\pi}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~e^{i m \pi}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(-1)^{m} \, , </math> </td> </tr> </table> </div> in which case, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~Q^m_{n-\frac{1}{2}}(\cosh\eta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \sqrt{\frac{\pi}{2}} ~\Gamma(n+m + \tfrac{1}{2}) ~(-1)^m\biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] P^{-n}_{-m - \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> </table> </div> ---- Now, since, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~P^\mu_\nu(z)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~P^\mu_{-\nu-1}(z) \, ,</math> </td> </tr> </table> </div> if we make the substitution, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~-(\nu + 1)</math> </td> <td align="center"> <math>~\rightarrow</math> </td> <td align="left"> <math>~-(m+\tfrac{1}{2})</math> </td> <td align="center"> <math>~\Rightarrow</math> </td> <td align="right"> <math>~\nu</math> </td> <td align="center"> <math>~\rightarrow</math> </td> <td align="left"> <math>~m - \tfrac{1}{2} \, ,</math> </td> </tr> </table> </div> we also know that, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~P^\mu_{m-\frac{1}{2}}(z)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~P^\mu_{-m-\frac{1}{2}}(z) \, .</math> </td> </tr> </table> </div> <span id="QPrelation">Hence, we can write,</span> <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~Q^m_{n-\frac{1}{2}}(\cosh\eta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \sqrt{\frac{\pi}{2}} ~\Gamma(n+m + \tfrac{1}{2}) ~(-1)^m\biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] P^{-n}_{m - \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> </table> </div> ---- Finally, another relation states that, for <math>~n \in \mathbb{N}_0</math>, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~P^{-n}_{m-\frac{1}{2}}(z)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ \frac{\Gamma(m-n+\frac{1}{2})}{\Gamma(m+n+\frac{1}{2})} \biggr] P^n_{m-\frac{1}{2}}(z) \, .</math> </td> </tr> </table> </div> So, we obtain, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~Q^m_{n-\frac{1}{2}}(\cosh\eta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(-1)^m \sqrt{\frac{\pi}{2}} ~\Gamma(n+m + \tfrac{1}{2}) \biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] \biggl[ \frac{\Gamma(m-n+\frac{1}{2})}{\Gamma(m+n+\frac{1}{2})} \biggr]P^{n}_{m - \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(-1)^m \sqrt{\frac{\pi}{2}} ~\Gamma(m-n+\tfrac{1}{2}) \biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] P^{n}_{m - \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> </table> </div> This matches expressions #2 and #3, above. ==Index Values of Zero== Setting <math>~n = m = 0</math> gives the following sought-for relationship: <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~Q^0_{-\frac{1}{2}}(\cosh\eta)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \sqrt{\frac{\pi}{2}} ~\Gamma(\tfrac{1}{2}) \biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] P^{0}_{- \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{\pi}{\sqrt{2}} ~ \biggl[ \frac{1}{ \sqrt{\sinh\eta}} \biggr] P^{0}_{- \frac{1}{2}} (\coth\eta) \, . </math> </td> </tr> </table> </div> ==Joel's Additional Manipulations== From [https://dlmf.nist.gov/14.19.iv §14.19.6 of DLMF], we find the following summation expression: <div align="center"> <math>~\boldsymbol{Q}^{\mu}_{-\frac{1}{2}}\left(\cosh\xi\right)+2\sum_{n=1}^{\infty} \frac{\Gamma\left(\mu+n+\tfrac{1}{2}\right)}{\Gamma\left(\mu+\tfrac{1}{2} \right)}\boldsymbol{Q}^{\mu}_{n-\frac{1}{2}}\left(\cosh\xi\right)\cos\left(n \phi\right)=\dfrac{\left(\frac{1}{2}\pi\right)^{1/2}\left(\sinh\xi\right)^{\mu }}{\left(\cosh\xi-\cos\phi\right)^{\mu+(1/2)}} </math></div> Then, if we again employ the [http://dlmf.nist.gov/14.3.E10 DLMF relationship between '''bold''' and plain-text function names], namely, <div align="center"> <math> \boldsymbol{Q}^{\mu}_{n-\frac{1}{2}}\left(x\right) = e^{-\mu\pi i}\frac{Q^{\mu}_{n-\frac{1}{2}}\left(x\right)}{\Gamma\left(\mu+n + \tfrac{1}{2} \right)} \, , </math> </div> where we have made the substitution, <math>~\nu \rightarrow (n-\tfrac{1}{2})</math>, the ''Sums'' expression becomes, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~e^{-\mu\pi i}\frac{Q^{\mu}_{-\frac{1}{2}}\left(\cosh\xi\right)}{\Gamma\left(\mu+ \tfrac{1}{2} \right)}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \dfrac{\left(\frac{1}{2}\pi\right)^{1/2}\left(\sinh\xi\right)^{\mu }}{\left(\cosh\xi-\cos\phi\right)^{\mu+(1/2)}} - 2\sum_{n=1}^{\infty} \frac{\Gamma\left(\mu+n+\tfrac{1}{2}\right)}{\Gamma\left(\mu+\tfrac{1}{2} \right)} \biggl[ e^{-\mu\pi i}\frac{Q^{\mu}_{n-\frac{1}{2}}\left(\cosh\xi\right)}{\Gamma\left(\mu+n + \tfrac{1}{2} \right)} \biggr] \cos\left(n \phi\right) </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~Q^{\mu}_{-\frac{1}{2}}\left(\cosh\xi\right)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ e^{\mu\pi i} \Gamma\left(\mu+ \tfrac{1}{2} \right) \biggl[ \dfrac{\left(\frac{1}{2}\pi\right)^{1/2}\left(\sinh\xi\right)^{\mu }}{\left(\cosh\xi-\cos\phi\right)^{\mu+(1/2)}}\biggr] - 2\sum_{n=1}^{\infty} Q^{\mu}_{n-\frac{1}{2}}\left(\cosh\xi\right) \cos\left(n \phi\right) \, . </math> </td> </tr> </table> </div> When dealing with Dyson-Wong tori, we will set <math>~\mu = 0</math>, in which case the ''Sums'' expression becomes, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~Q_{-\frac{1}{2}}\left(\cosh\xi\right)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \dfrac{ \pi/\sqrt{2} }{\left(\cosh\xi-\cos\phi\right)^{\frac{1}{2}} }\biggr] - 2\sum_{n=1}^{\infty} Q_{n-\frac{1}{2}}\left(\cosh\xi\right) \cos\left(n \phi\right) \, . </math> </td> </tr> </table> </div> But this can be rewritten in the form, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \sum_{n=0}^{\infty} \epsilon_n Q_{n-\frac{1}{2}}\left(\cosh\xi\right) \cos\left(n \phi\right) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \dfrac{ \pi/\sqrt{2} }{\left(\cosh\xi-\cos\phi\right)^{\frac{1}{2}} }\biggr] </math> </td> </tr> </table> </div>
Summary:
Please note that all contributions to JETohlineWiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
JETohlineWiki:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Navigation menu
Personal tools
Not logged in
Talk
Contributions
Log in
Namespaces
Page
Discussion
English
Views
Read
Edit
View history
More
Search
Navigation
Main page
Tiled Menu
Table of Contents
Old (VisTrails) Cover
Appendices
Variables & Parameters
Key Equations
Special Functions
Permissions
Formats
References
lsuPhys
Ramblings
Uploaded Images
Originals
Recent changes
Random page
Help about MediaWiki
Tools
What links here
Related changes
Special pages
Page information