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<div style="direction: ltr;font-family: Tahoma;color: #000000;font-size: 10pt;">Thanks John.<br>
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<div style="direction: ltr;" id="divRpF168337"><font face="Tahoma" color="#000000" size="2"><b>From:</b> General [general-bounces+john.williamson=glasgow.ac.uk@lists.natureoflightandparticles.org] on behalf of John Duffield [johnduffield@btconnect.com]<br>
<b>Sent:</b> Friday, November 20, 2015 6:06 PM<br>
<b>To:</b> 'Nature of Light and Particles - General Discussion'<br>
<b>Subject:</b> Re: [General] High impact publications<br>
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<p class="MsoNormal"><span style="font-size:11.0pt; color:#1F497D">I volunteer to do some proofreading. </span></p>
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<p class="MsoNormal"><b><span style="font-size:11.0pt" lang="EN-US">From:</span></b><span style="font-size:11.0pt" lang="EN-US"> General [mailto:general-bounces+johnduffield=btconnect.com@lists.natureoflightandparticles.org]
<b>On Behalf Of </b>John Williamson<br>
<b>Sent:</b> 20 November 2015 17:47<br>
<b>To:</b> Nature of Light and Particles - General Discussion <general@lists.natureoflightandparticles.org><br>
<b>Subject:</b> [General] High impact publications</span></p>
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<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Dear All,</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="color:black" lang="EN-US"> </span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Over the last decade or so Martin and I have submitted over a dozen papers to the peer reviewed press without any success.</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">I would like to try again with a paper, perhaps to Phys. Rev, on the new theory. I’m looking for several things.</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="color:black" lang="EN-US"> </span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Firstly, a proof reading of the manuscript, This is more especially to pick up things that are not clear in the explanation of the science – not the English.</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="color:black" lang="EN-US"> </span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Secondly – suggestions of which journal might be appropriate. The manuscript will be about 30 pages in pre-print form. I’ve included a title and abstract of
the first draft below for information.</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="color:black" lang="EN-US"> </span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Thirdly – I understand that it is now the done thing to “help the editor” by suggesting appropriate referees. I have never done this before, so advice on whether
to do this at all, appropriate people and the right way to do this would be appreciated.</span><span style="color:black" lang="EN-US"></span></p>
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<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Regards, John.</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="color:black" lang="EN-US"> </span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">Root-energy in space and time</span><a name="_GoBack"></a><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black">A relativistic formalism is developed to describe a dynamical square-root energy density transforming within a set of space-time forms. A minimal formalism
to describe the process is adopted, with as few starting parameters as possible. The simplest general linear equation within this model is derived. A restriction to the bi-vector forms alone has a structure which parallels the free-space Maxwell equations.
Allowed solutions of this subset are quantised in that they represent the exchange of a packet of energy. Including a (square root) invariant mass density leads to new kinds of solutions which are re-circulating within momentum-space and exhibit an intrinsically
fermionic 720 degree symmetry. Comparisons are made between the solutions of the new model and the physical properties of the photon, electron and positron.
</span><span style="color:black" lang="EN-US"></span></p>
<p class="MsoNormal" style=""><span style="font-size:10.0pt; font-family:"Times",serif; color:black"> </span><span style="color:black" lang="EN-US"></span></p>
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