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X-WR-CALNAME;VALUE=TEXT:ITC Colloquium
PRODID:-//Harvard events data//EN
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UID:event_1593076_0
SUMMARY:ITC Colloquium
DESCRIPTION:<p dir="ltr" style="margin-top:0pt;margin-bottom:0pt">	<span style="caret-color:#222222"><span style="color:#222222"><span style="Helvetica,sans-serif"><span style="line-height:1.38"><font size="4"><span style="color:#000000"><span style="font-variant-ligatures:normal"><span style="font-variant-east-asian:normal"><span style="vertical-align:baseline"><span style="white-space:pre-wrap"><strong>ITC Colloquium– </strong></span></span></span></span></span><span style="color:#000000"><strong>Monica Gallegos-Garcia</strong></span></font></span></span></span></span></p><p style="margin-top:0pt;margin-bottom:9pt">	<span><span style="color:#000000"><span style='newroman",serif'><span style="line-height:1.38"><span style="font-variant-ligatures:normal"><span style="font-variant-east-asian:normal"><span style="vertical-align:baseline"><span style="white-space:pre-wrap">Phillips and streamed: </span></span></span></span><a data-saferedirecturl="https://www.google.com/url?q=https://youtube.com/live/5Et9oAeMEr4&amp;source=gmail&amp;ust=1725974208992000&amp;usg=AOvVaw2RYJv0AoYoUCOpMeciWDPy" href="https://youtube.com/live/5Et9oAeMEr4" style="color:#1155cc;" target="_blank">https://youtube.com/live/<wbr></wbr>5Et9oAeMEr4</a></span></span></span></span></p><p dir="ltr" style="margin-top:0pt;margin-bottom:9pt">	<span style="caret-color:#222222"><span style="color:#222222"><span style="Helvetica,sans-serif"><span style="line-height:1.38"><strong style="text-align:justify">"Gaining insights into the formation of binary black hole mergers: Towards a new era of binary evolution"</strong></span></span></span></span></p><p dir="ltr" style="text-align:justify;margin-top:0pt;margin-bottom:0pt">	<span style="caret-color:#222222"><span style="color:#222222"><span style="Helvetica,sans-serif"><span style="line-height:1.38"><span style="font-variant-ligatures:normal"><span style="font-variant-alternates:normal"><span style="font-variant-numeric:normal"><span style="font-variant-east-asian:normal"><span style="vertical-align:baseline"><span style="white-space:pre-wrap"><font face="trebuchet ms, sans-serif"><font color="#000000">The detections of binary black hole mergers through gravitational waves have revolutionized astronomy. Today, most theoretical models of their formation rely on a set of tools developed more than 20 years ago. Although these codes have been instrumental for our general understanding of merging compact objects, most rely on analytical fits of single-star evolutionary tracks and parameterized models for interactive phases of binary evolution. Simultaneously, we are experiencing a rise in the number of merger detections, and with the advent of next-generation instruments, this number will increase 1000-fold, revealing a larger, more diverse population. In this talk I will show how using detailed, state-of-the-art MESA simulations and physically-motivated models can affect the orbital period evolution of binary systems, the predicted formation paths of merging binary black holes, and consequently their merger rates. I will also describe how exploring key electromagnetically-observed binary systems allows us to more comprehensively study the formation histories of gravitational wave sources.</font></font></span></span></span></span></span></span></span></span></span></span></p>
LOCATION:Phillips Auditorium
STATUS:CONFIRMED
DTSTART:20240912T150000Z
DTEND:20240912T160000Z
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