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    <p><b style="font-weight:normal;"
        id="docs-internal-guid-c411744a-c30c-f387-de7b-85ed6c2f6e35">Estimados,<br>
        <br>
        Les recordamos que </b><span style="font-weight:normal;">hoy
        miércoles se llevará a cabo la siguiente charla en la Sala del
        IALP a las 12:00 hs.</span><b style="font-weight:normal;"
        id="docs-internal-guid-c411744a-c30c-f387-de7b-85ed6c2f6e35"><br>
        <br>
        --<br>
        Secretaría de Ciencia y Técnica<br>
        FCAG</b></p>
    <p><b style="font-weight:normal;"
        id="docs-internal-guid-c411744a-c30c-f387-de7b-85ed6c2f6e35"><b>-------------------------------------------------------------------------------------------------------------------------------------------------</b></b><br>
      <b style="font-weight:normal;"
        id="docs-internal-guid-c411744a-c30c-f387-de7b-85ed6c2f6e35"><b><b
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            id="docs-internal-guid-f1cc35e4-6fbc-dc7e-daf7-c404810f4f97">
            <p dir="ltr"
              style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align:
              justify;"><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Seminario:</span><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;"> Dr. Clement Stahl </span></p>
            <p dir="ltr"
              style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align:
              justify;"><span style="font-size:12pt;font-family:Verdana;color:#212121;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Pontificia Universidad Católica de Valparaíso</span></p>
            <br>
            <p dir="ltr"
              style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align:
              justify;"><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:underline;-webkit-text-decoration-skip:none;text-decoration-skip-ink:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Título</span><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">:</span><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">  Charged cosmological black hole.</span></p>
            <br>
            <p dir="ltr"
              style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align:
              justify;"><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:underline;-webkit-text-decoration-skip:none;text-decoration-skip-ink:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Resumen:</span><span style="font-size:12pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;"> The cosmological black holes are black holes living not in an asymptotically flat universe but in an expanding spacetime. They have a rich dynamics in particular for their mass and horizon. In this presentation, we perform a natural step in investigating this new type of black hole: we consider the possibility of a charged cosmological black hole. We derive the general equations of motion governing its dynamics and report a new analytic solution for the special case of the charged Lematre-Tolman-Bondi equations of motion that describe a charged cosmological black hole. We then study various relevant quantities for the characterization of the black hole such as the C-function, the effect of the charge on the black hole flux and the nature of the singularity. We also perform numerical investigations to strengthen our results. Finally we challenge a model of gamma ray burst within our framework.</span></p>
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