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Hi again,
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<div class="">Of course, I forgot to add the speakers name in the announcement, my apologies. </div>
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<div class="">He is <b class="">Joshua Ziegler</b>, PhD student visiting from the university of Texas. </div>
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<div class="">Best regards, </div>
<div class="">Ana<br class="">
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<div class="">On 7 Nov 2022, at 23:49, Ana Sagués Carracedo <<a href="mailto:ana.sagues-carracedo@fysik.su.se" class="">ana.sagues-carracedo@fysik.su.se</a>> wrote:</div>
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Dear all,
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<div class="">We are having an Extreme Object meeting <b class="">this week on Thursday 10th November
</b>at 13:15 in the <b class="">Mega room</b> (6th floor, house 3, where Nordita). </div>
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<div class="">Our speaker is Katie Freeze’s PhD student visiting us from Texas. He will stay around until the end of the month and will present some of his work to us. </div>
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<div class="">Following tittle and abstract:</div>
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<div style="text-align: center;" class=""><font class=""><span style="caret-color: rgb(0, 0, 0);" class=""><b class="">Dark Matter Annihilation in Stars: A New Lease on Life?</b></span></font></div>
<div class=""><span style="caret-color: rgb(0, 0, 0);" class=""><b class=""><br class="">
</b></span></div>
<div style="text-align: center;" class=""><span style="caret-color: rgb(0, 0, 0);" class="">What happens to a star when fusion isn't the only relevant power source? We explore how introducing non-nuclear energy, such as energy that could come from dark matter
annihilation, affects the evolution of massive stars. In particular, we aim to determine whether stars which produce a significant amount of energy from non-nuclear sources can avoid undergoing pair instability supernovae, and can therefore form black holes
in the forbidden mass gap between 50 and 140 Msun.</span></div>
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<div class=""><span style="caret-color: rgb(0, 0, 0);" class="">Looking forward to see you in a couple of days, </span></div>
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<div class=""><font class=""><span style="caret-color: rgb(0, 0, 0);" class="">Kind regards, </span></font></div>
<div class=""><font class="">Ana Sagués Carracedo & Haakon Andresen</font></div>
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<a href="mailto:okc-wp4@albanova.se" class="">okc-wp4@albanova.se</a> mailing list</div>
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