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For your info.<br>
Volker<br>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">Subject:
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<td>radiative Moeller scattering</td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">Date: </th>
<td>Thu, 25 Feb 2016 08:09:38 -0500</td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">From: </th>
<td>burkert <a class="moz-txt-link-rfc2396E" href="mailto:burkert@jlab.org"><burkert@jlab.org></a></td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">To: </th>
<td><a class="moz-txt-link-abbreviated" href="mailto:clas12_high_luminosity@jlab.org">clas12_high_luminosity@jlab.org</a></td>
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<pre>Dear all,
See this link: <a class="moz-txt-link-freetext" href="http://arxiv.org/abs/1602.07609">http://arxiv.org/abs/1602.07609</a>. It deals with the
radiative Moller calculations in NLO. This is the process I keep
pestering everyone with. It appears the process has never before been
properly computed in the non ultra-relativistic limit, which is relevant
to our background processes. They advertize a code they will develop.
Maybe it will be useful for us.
Volker
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