<div dir="ltr"><br><br><div class="gmail_quote">On Tue, Aug 25, 2009 at 11:25 AM, Oleg Goldshmidt <span dir="ltr">&lt;<a href="mailto:pub@goldshmidt.org">pub@goldshmidt.org</a>&gt;</span> wrote:<br><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex;">
<div class="im">On Tue, Aug 25, 2009 at 10:40 AM, Gilad Ben-Yossef&lt;<a href="mailto:gilad@codefidence.com">gilad@codefidence.com</a>&gt; wrote:<br>
&gt; Oleg Goldshmidt wrote:<br>
&gt;<br>
&gt; Once you have satisfied yourself that N=3, you can derive R^-2 easily<br>
&gt; from flux considerations.<br>
&gt;<br>
&gt;<br>
&gt; Until, of course, the invention of the flux capacitor...<br>
&gt;<br>
&gt;  <a href="http://en.wikipedia.org/wiki/DeLorean_time_machine" target="_blank">http://en.wikipedia.org/wiki/DeLorean_time_machine</a><br>
<br>
</div>Oh, anything is possible if you travel through space-time in a<br>
DeLorean... In particular, when you travel close to the speed of light<br>
you emit mostly in the forward direction, not isotropically...<br>
<br>
;-)<br>
<div><div></div><div class="h5"></div></div></blockquote><div>&quot;when you travel close to the speed of light&quot;</div><div> </div><div>88 Miles per hour?</div><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex;">
<div><div class="h5"><br>
--<br>
Oleg Goldshmidt | <a href="mailto:oleg@goldshmidt.org">oleg@goldshmidt.org</a><br>
<br>
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