<html><body><div style="color:#000; background-color:#fff; font-family:HelveticaNeue, Helvetica Neue, Helvetica, Arial, Lucida Grande, sans-serif;font-size:16px"><div id="yui_3_16_0_1_1443407971651_3164"><span id="yui_3_16_0_1_1443407971651_4355">Rich, John W, Martin and all,</span></div><div id="yui_3_16_0_1_1443407971651_3164"><br></div><div id="yui_3_16_0_1_1443407971651_3164" dir="ltr"><span id="yui_3_16_0_1_1443407971651_3575" class="">Two papers </span>may be of interest to those building or refining electron models, especially those with early universe electron models. These papers are about to be published in Physics Review Letters .</div><div id="yui_3_16_0_1_1443407971651_3164"><span><br></span></div><div id="yui_3_16_0_1_1443407971651_3164" dir="ltr"><span id="yui_3_16_0_1_1443407971651_4013">From LLNL, </span><a href="https://www.llnl.gov/news/new-stealth-dark-matter-theory-may-explain-mystery-universes-missing-mass" id="yui_3_16_0_1_1443407971651_4108">New 'stealth dark matter' theory may explain mystery of the universe's missing mass</a> </div><div id="yui_3_16_0_1_1443407971651_3164" dir="ltr"><br></div><div id="yui_3_16_0_1_1443407971651_3164" dir="ltr"><font size="2" id="yui_3_16_0_1_1443407971651_3797" style="color: rgb(51, 51, 51); font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px;">Through a combination of computer simulations and theoretical results, researchers Pavlos Vranas and colleagues (editor's note: Applequist et al) have now developed a "stealth dark matter" model that could help unravel the mystery of why dark matter behaves like it does, what particles make it up, and what force binds them. Crucially, the model offers assumptions that physicists should be able to test using CERN's <a href="http://www.gizmag.com/tag/large-hadron-collider/" target="_blank" style="border: 0px; font-family: inherit; font-style: inherit; font-variant: inherit; line-height: inherit; vertical-align: baseline; color: rgb(30, 141, 215); text-decoration: none;" id="yui_3_16_0_1_1443407971651_3703" class="">Large Hadron Collider</a> (LHC) particle accelerator. </font><span id="yui_3_16_0_1_1443407971651_3941" style="color: rgb(51, 51, 51); font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px; font-size: small;">The stealth dark matter model predicts that dark matter is stable, but also produces large quantities of electrically charged, unstable nuclear particles. These short-lived particles, now long decayed, would have left a definite mark in the very early universe, with the extremely high</span><span style="color: rgb(51, 51, 51); font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px; font-size: small;" id="yui_3_16_0_1_1443407971651_4354"> </span><a href="https://en.wikipedia.org/wiki/Plasma_(physics)" target="_blank" id="yui_3_16_0_1_1443407971651_3707" class="" style="font-family: inherit; line-height: inherit; border: 0px; font-style: inherit; font-variant: inherit; vertical-align: baseline; color: rgb(30, 141, 215); text-decoration: none;">plasma</a><span style="color: rgb(51, 51, 51); font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px; font-size: small;"> </span><span style="color: rgb(51, 51, 51); font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px; font-size: small;" id="yui_3_16_0_1_1443407971651_4297">temperatures forcing them to interact with ordinary matter. </span></div><div style="margin-bottom: 20px; border: 0px; font-family: ProximaNova, 'Helvetica Neue', Arial; line-height: 26px; vertical-align: baseline; color: rgb(51, 51, 51);" id="yui_3_16_0_1_1443407971651_3701" class="" dir="ltr"><span id="yui_3_16_0_1_1443407971651_3855"><font size="3" id="yui_3_16_0_1_1443407971651_4427"><b id="yui_3_16_0_1_1443407971651_3884"><font id="yui_3_16_0_1_1443407971651_3883">"These interactions in the early universe are important because ordinary and dark matter abundances today are strikingly similar in size</font></b><font id="yui_3_16_0_1_1443407971651_3886">, suggesting this occurred because of a balancing act performed between the two before the universe cooled," says Vranas.</font></font></span></div><dt style="font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3399" class=""><br></dt><dt style="font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3399" class=""><br></dt><dt style="font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3399" class="">1. <span class="" style="font-weight: bold;" id="yui_3_16_0_1_1443407971651_3401"><a href="http://arxiv.org/abs/1503.04205" title="Abstract" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3403" class="" title-off="">arXiv:1503.04205</a> [<a href="http://arxiv.org/pdf/1503.04205" title="Download PDF" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3405" class="" title-off="">pdf</a>, <a href="http://arxiv.org/format/1503.04205" title="Other formats" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3407" class="" title-off="">other</a>]</span></dt><dd style="padding-bottom: 1em; font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3409" class=""><div class="" style="line-height: 18.719999313354492px;" id="yui_3_16_0_1_1443407971651_3411"><div class="" style="font-size: large; font-weight: bold; margin: 0.25em 0px 0px; line-height: 21.600000381469727px;" id="yui_3_16_0_1_1443407971651_3413">Direct Detection of Stealth Dark Matter through Electromagnetic Polarizability</div><div class="" style="font-size: 16px;" id="yui_3_16_0_1_1443407971651_3415"><a href="http://arxiv.org/find/hep-ph/1/au:+Appelquist_T/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3417" class="">Thomas Appelquist</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Berkowitz_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3419" class="">Evan Berkowitz</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Brower_R/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3421" class="">Richard C. Brower</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Buchoff_M/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3423" class="">Michael I. Buchoff</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Fleming_G/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3425" class="">George T. Fleming</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Jin_X/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3427" class="">Xiao-Yong Jin</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kiskis_J/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3429" class="">Joe Kiskis</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kribs_G/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3431" class="">Graham D. Kribs</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Neil_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3433" class="">Ethan T. Neil</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Osborn_J/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3435" class="">James C. Osborn</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Rebbi_C/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3437" class="">Claudio Rebbi</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Rinaldi_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3439" class="">Enrico Rinaldi</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Schaich_D/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3441" class="">David Schaich</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Schroeder_C/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3443" class="">Chris Schroeder</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Syritsyn_S/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3445" class="">Sergey Syritsyn</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Vranas_P/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3447" class="">Pavlos Vranas</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Weinberg_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3449" class="">Evan Weinberg</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Witzel_O/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3451" class="">Oliver Witzel</a></div><div class="" style="font-size: 13px;" id="yui_3_16_0_1_1443407971651_3453"><span class="" style="display: inline;" id="yui_3_16_0_1_1443407971651_3455">Comments:</span> 6 pages, 2 figures, citations added, typos fixed, minor clarifications</div><div class="" style="font-size: 13px;" id="yui_3_16_0_1_1443407971651_3457"><span class="" style="display: inline;" id="yui_3_16_0_1_1443407971651_3459">Subjects:</span> <span class="" style="font-weight: bold;" id="yui_3_16_0_1_1443407971651_3461">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Physics - Lattice (hep-lat)</div><div class="" style="font-size: 13px;" id="yui_3_16_0_1_1443407971651_3457"><br></div><div class="" style="font-size: 13px;" id="yui_3_16_0_1_1443407971651_3457" dir="ltr"><span style="font-size: 14px; line-height: 20.15999984741211px;" id="yui_3_16_0_1_1443407971651_4818" class="">Full ABSTRACT: We calculate the spin-independent scattering cross section for direct detection that results from the electromagnetic polarizability of a composite scalar baryon dark matter candidate -- "Stealth Dark Matter", that is based on a dark SU(4) confining gauge theory. In the nonrelativistic limit, electromagnetic polarizability proceeds through a dimension-7 interaction leading to a very small scattering cross section for dark matter with weak scale masses. This represents a lower bound on the scattering cross section for composite dark matter theories with electromagnetically charged constituents. We carry out lattice calculations of the polarizability for the lightest baryons in SU(3) and SU(4) gauge theories using the background field method on quenched configurations. <b id="yui_3_16_0_1_1443407971651_5186"><i id="yui_3_16_0_1_1443407971651_5185">We find the polarizabilities of SU(3) and SU(4) to be comparable (within about 50%) normalized to the baryon mass, which is suggestive for extensions to larger SU(N) groups.</i></b> The resulting scattering cross sections with a xenon target are shown to be potentially detectable in the dark matter mass range of about 200-700 GeV, where the lower bound is from the existing LUX constraint while the upper bound is the coherent neutrino background. Significant uncertainties in the cross section remain due to the more complicated interaction of the polarizablity operator with nuclear structure, however the steep dependence on the dark matter mass, </span><span class="" style="color: rgb(136, 136, 136); font-size: 14px; line-height: 20.15999984741211px;" id="yui_3_16_0_1_1443407971651_4820"></span><span class="" id="MathJax-Element-1-Frame" role="textbox" aria-readonly="true" style="display: inline; line-height: normal; font-size: 14px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; border: 0px; padding: 0px; margin: 0px;"><nobr style="transition: none; -webkit-transition: none; border: 0px; padding: 0px; margin: 0px; max-width: 5000em; max-height: 5000em; vertical-align: 0px;" id="yui_3_16_0_1_1443407971651_4823" class=""><span class="" id="MathJax-Span-1" style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 2.517em;"><span style="transition: none; 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vertical-align: 0px; font-size: 12px; font-family: STIXGeneral-Regular;">^6 </span></span></span></span></span></span></span></span></nobr></span><span class="" role="textbox" aria-readonly="true" style="display: inline; line-height: normal; font-size: 14px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; border: 0px; padding: 0px; margin: 0px;" id="yui_3_16_0_1_1443407971651_4926"><nobr style="transition: none; -webkit-transition: none; border: 0px; padding: 0px; margin: 0px; max-width: 5000em; max-height: 5000em; vertical-align: 0px;" class="" id="yui_3_16_0_1_1443407971651_4925"><span class="" style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 2.517em;" id="yui_3_16_0_1_1443407971651_4924"><span style="transition: none; -webkit-transition: none; display: inline-block; position: relative; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 2.101em; 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width: 0px; min-height: 2.042em;" id="yui_3_16_0_1_1443407971651_4851" class=""></span></span></span></span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 0px; min-height: 2.509em;" id="yui_3_16_0_1_1443407971651_4853" class=""></span></span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border-width: 0px 0px 0px 0em; border-left-style: solid; padding: 0px; margin: 0px; vertical-align: -0.423em; overflow: hidden; width: 0px; min-height: 1.49em;" id="yui_3_16_0_1_1443407971651_4855" class=""></span></span></nobr></span><span id="yui_3_16_0_1_1443407971651_4857" class="" style="font-size: 14px; line-height: 20.15999984741211px;">, suggests the observable dark matter mass range is not appreciably modified. We briefly highlight collider searches for the mesons in the theory as well as the indirect astrophysical effects that may also provide excellent probes of stealth dark matter.</span></div></div></dd><dt style="font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3463" class="">2. <span class="" style="font-weight: bold;" id="yui_3_16_0_1_1443407971651_3465"><a href="http://arxiv.org/abs/1503.04203" title="Abstract" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3467" class="" title-off="">arXiv:1503.04203</a> [<a href="http://arxiv.org/pdf/1503.04203" title="Download PDF" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3469" class="" title-off="">pdf</a>, <a href="http://arxiv.org/format/1503.04203" title="Other formats" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3471" class="" title-off="">other</a>]</span></dt><dd style="padding-bottom: 1em; font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-size: 14px;" id="yui_3_16_0_1_1443407971651_3473" class=""><div class="" style="line-height: 18.719999313354492px;" id="yui_3_16_0_1_1443407971651_3475"><div class="" style="font-size: large; font-weight: bold; margin: 0.25em 0px 0px; line-height: 21.600000381469727px;" id="yui_3_16_0_1_1443407971651_3477">Stealth Dark Matter: Dark scalar baryons through the Higgs portal</div><div class="" style="font-size: 16px;" id="yui_3_16_0_1_1443407971651_3479"><a href="http://arxiv.org/find/hep-ph/1/au:+Appelquist_T/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3481" class="">Thomas Appelquist</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Brower_R/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3483" class="">Richard C. Brower</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Buchoff_M/0/1/0/all/0/1" id="yui_3_16_0_1_1443407971651_3485" class="">Michael I. Buchoff</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Fleming_G/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3487" class="">George T. Fleming</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Jin_X/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3489" class="">Xiao-Yong Jin</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kiskis_J/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3491" class="">Joe Kiskis</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kribs_G/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3493" class="">Graham D. Kribs</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Neil_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3495" class="">Ethan T. Neil</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Osborn_J/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3497" class="">James C. Osborn</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Rebbi_C/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3499" class="">Claudio Rebbi</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Rinaldi_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3501" class="">Enrico Rinaldi</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Schaich_D/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3503" class="">David Schaich</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Schroeder_C/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3505" class="">Chris Schroeder</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Syritsyn_S/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3507" class="">Sergey Syritsyn</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Vranas_P/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3509" class="">Pavlos Vranas</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Weinberg_E/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3511" class="">Evan Weinberg</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Witzel_O/0/1/0/all/0/1" style="text-decoration: none;" id="yui_3_16_0_1_1443407971651_3513" class="">Oliver Witzel</a></div><div class="" style="font-size: 13px;" id="yui_3_16_0_1_1443407971651_3515"><span class="" style="display: inline;" id="yui_3_16_0_1_1443407971651_3517">Comments:</span> 15 pages, 3 figures, citations added, typos fixed, minor clarifications</div><div class="" style="font-size: 13px;" dir="ltr" id="yui_3_16_0_1_1443407971651_3519"><span class="" style="display: inline;" id="yui_3_16_0_1_1443407971651_3521">Subjects:</span> <span class="" style="font-weight: bold;" id="yui_3_16_0_1_1443407971651_3523">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Physics - Lattice (hep-lat)</div><div class="" style="font-size: 13px;" dir="ltr" id="yui_3_16_0_1_1443407971651_3519"><span id="yui_3_16_0_1_1443407971651_5053" class="" style="font-size: 14px; line-height: 20.15999984741211px;">ABSTRACT QUOTE: We present a new model of "Stealth Dark Matter": a composite baryonic scalar of an </span><span class="" id="yui_3_16_0_1_1443407971651_5055" style="color: rgb(136, 136, 136); font-size: 14px; line-height: 20.15999984741211px;"></span><span class="" id="MathJax-Element-1-Frame" role="textbox" aria-readonly="true" style="display: inline; line-height: normal; font-size: 14px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; border: 0px; padding: 0px; margin: 0px;"><nobr style="transition: none; -webkit-transition: none; border: 0px; padding: 0px; margin: 0px; max-width: 5000em; max-height: 5000em; vertical-align: 0px;" id="yui_3_16_0_1_1443407971651_5058" class=""><span class="" id="MathJax-Span-1" style="transition: none; 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width: 0.06em;" id="yui_3_16_0_1_1443407971651_5079" class=""></span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 0px; min-height: 2.509em;" id="yui_3_16_0_1_1443407971651_5081" class=""></span></span><span style="transition: none; -webkit-transition: none; ; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; top: -1.892em; left: 0.699em;" id="yui_3_16_0_1_1443407971651_5083" class=""><span class="" id="MathJax-Span-8" style="transition: none; -webkit-transition: none; display: inline; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; font-size: 12px; font-family: STIXGeneral-Italic;">D</span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 0px; min-height: 2.042em;" id="yui_3_16_0_1_1443407971651_5086" class=""></span></span></span></span><span class="" id="MathJax-Span-9" style="transition: none; -webkit-transition: none; display: inline; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; font-family: STIXGeneral-Regular;">)</span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 0px; min-height: 2.509em;" id="yui_3_16_0_1_1443407971651_5089" class=""></span></span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border-width: 0px 0px 0px 0em; border-left-style: solid; padding: 0px; margin: 0px; vertical-align: -0.28em; overflow: hidden; width: 0px; min-height: 1.154em;" id="yui_3_16_0_1_1443407971651_5091" class=""></span></span></nobr></span><span id="yui_3_16_0_1_1443407971651_5093" class="" style="font-size: 14px; line-height: 20.15999984741211px;"> strongly-coupled theory with even </span><span class="" id="yui_3_16_0_1_1443407971651_5095" style="color: rgb(136, 136, 136); 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position: static; border: 0px; padding: 0px; margin: 0px; vertical-align: 0px; width: 0px; min-height: 2.509em;" id="yui_3_16_0_1_1443407971651_5123" class=""></span></span></span><span style="transition: none; -webkit-transition: none; display: inline-block; position: static; border-width: 0px 0px 0px 0em; border-left-style: solid; padding: 0px; margin: 0px; vertical-align: -0.248em; overflow: hidden; width: 0px; min-height: 1.122em;" id="yui_3_16_0_1_1443407971651_5125" class=""></span></span></nobr></span><span id="yui_3_16_0_1_1443407971651_5127" class="" style="font-size: 14px; line-height: 20.15999984741211px;">.</span></div></div></dd><div id="yui_3_16_0_1_1443407971651_3164"><span id="yui_3_16_0_1_1443407971651_5356">Best Regards,</span></div><div id="yui_3_16_0_1_1443407971651_3164"><span><br></span></div><div id="yui_3_16_0_1_1443407971651_3164"><span><br></span></div><div id="yui_3_16_0_1_1443407971651_3164"><span id="yui_3_16_0_1_1443407971651_4562">David</span></div><blockquote style="border-left: 2px solid rgb(16, 16, 255); margin-left: 5px; margin-top: 5px; padding-left: 5px;" id="yui_3_16_0_1_1443407971651_3377"><div style="font-family: HelveticaNeue, Helvetica Neue, Helvetica, Arial, Lucida Grande, sans-serif; font-size: 16px;" id="yui_3_16_0_1_1443407971651_3376"><div style="font-family: HelveticaNeue, Helvetica Neue, Helvetica, Arial, Lucida Grande, sans-serif; font-size: 16px;" id="yui_3_16_0_1_1443407971651_3375"><div class="y_msg_container" id="yui_3_16_0_1_1443407971651_3379"><br></div> </div> </div> </blockquote> </div></body></html>