<div dir="ltr"><p style="text-align:left;font-family:Verdana,Geneva,sans-serif"><strong>Estimados:</strong></p><p style="text-align:left;font-family:Verdana,Geneva,sans-serif"><strong>Agradecemos la difusión del <span class="">anuncio</span> del <span class="">seminario</span> que se dictará hoy, dentro del C<strong>iclo de Coloquios y <span class="">Seminarios</span> que se organizan en el Instituto de Física La Plata</strong>/ <strong>Departamento de Física.</strong></strong></p><p class="MsoNormal" align="center" style="text-align:center"><b><u><span lang="ES" style="font-family:Arial,sans-serif"><br></span></u></b></p><p class="MsoNormal" align="center" style="text-align:center"><b><u><span lang="ES" style="font-family:Arial,sans-serif">SEMINARIOS  DEL
IFLP y DEL DEPARTAMENTO  </span></u></b></p><p class="MsoNormal" align="center" style="text-align:center"><b><u><span lang="ES" style="font-family:Arial,sans-serif">MARTES 3 de MAYO
a las 11hs. </span></u></b></p><p class="MsoNormal" align="center" style="text-align:center"><b><u><span lang="EN-US" style="font-family:Arial,sans-serif">AULA CHICA</span></u></b></p><p class="MsoNormal" align="center" style="text-align:center"><span lang="PT-BR" style="font-family:Arial,sans-serif"><br>
<br>
</span><b><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black;background-image:initial;background-repeat:initial"></span></b></p><p class="MsoNormal" style="background-image:initial;background-repeat:initial"><b><u><span lang="EN-US" style="font-family:Arial,sans-serif">TÍTULO:</span></u></b><b><span lang="EN-US" style="font-family:Arial,sans-serif"> </span></b><b><span lang="EN-US" style="font-family:Arial,sans-serif"><font size="4">New Approaches to
Dark Matter</font></span></b></p><p class="MsoNormal" style="background-image:initial;background-repeat:initial"><b><span lang="EN-US" style="font-family:Arial,sans-serif"><br></span></b></p><p class="MsoNormal"><b><u><span lang="EN-US" style="font-family:Arial,sans-serif">EXPONE</span></u></b><b><span lang="EN-US" style="font-family:Arial,sans-serif;color:black">:</span></b><b><span lang="EN-US" style="font-family:Arial,sans-serif"> </span></b><font size="4"><b><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black;background-image:initial;background-repeat:initial">James Unwin</span></b><b><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black;background-image:initial;background-repeat:initial"></span></b></font></p><p class="MsoNormal"><b><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black;background-image:initial;background-repeat:initial"><font size="4">Department of Physics, University of Illinois at Chicago</font></span></b></p><pre style="text-align:center"><b><span lang="EN-US" style="font-family:Arial,sans-serif"> </span></b></pre><p class="MsoNormal" style="background-image:initial;background-repeat:initial"><b><u><span lang="PT-BR" style="font-family:Arial,sans-serif">Resumen:</span></u></b><span lang="PT-BR" style="font-family:Arial,sans-serif;color:black">
</span><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black">The presence of
dark matter provides a striking indication that the Standard Model can not
fully describe the physical Universe. I will first briefly outline the
evidence for dark matter and the traditional picture of </span><span lang="EN-US" style="font-family:Calibri,sans-serif;color:rgb(84,84,84);background-image:initial;background-repeat:initial"> </span><span lang="EN-US" style="font-family:Calibri,sans-serif;color:black">WIMP¹
dark matter. Notably, this dark matter scenario can be effectively
constrained via direct detection experiments and the LHC searches as I
will discuss. Subsequently, I shall highlight some distinct alternatives
to WIMPs for which these experimental limits are avoided or relaxed.
Specifically, I will outline models of "Freeze-in",
"Asymmetric Dark Matter", and "Flooded Dark Matter". These
alternative scenarios give a very different picture of cosmology and have
distinct signals and constraints compared to WIMP dark matter.</span></p><p style="font-family:Verdana,Geneva,sans-serif">



















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