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<title>PhTh-FI-ULB - Week of 10/25/2026</title>
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<title>Mon Oct 26 2026: ULB PhysTH Seminar, Felix Kahlhoefer [KIT, Karlsruhe],  [BEL-center:pheno]</title>
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<description>Mon Oct 26 2026 2:00 PM: &lt;b&gt;Dark matter from phase transitions - phase transitions from dark matter&lt;/b&gt;I will present the intriguing interplay between cosmological phase transitions and the out-of-equilibrium production of dark matter. If dark matter is produced non-thermally via non-renormalisable interactions (so-called UV-dominated freeze-in), the resulting abundance depends sensitively on the entire cosmological history. In particular, it can be strongly affected by cosmological first-order phase transition, after which the decaying scalar field transfers its energy density to the SM radiation and dilutes pre-existing particle abundances. I will discuss how this phase-in mechanism introduces a dependence of the final DM abundance on the details of the phase transition, in particular the subsequent equation of state of the universe. Using results from lattice simulations, I will show that the collision of highly-relativistic bubble walls leads to an equation of state that may differ significantly fro</description>
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<title>Tue Oct 27 2026: Lecture on "Modern Bayesian Inference" - B. Zaldívar [IFIC, Valencia]</title>
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