<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE rss PUBLIC "-//Netscape Communications//DTD RSS 0.91//EN" "http://my.netscape.com/publish/formats/rss-0.91.dtd">
<rss version="0.91">
<channel>
<title>BEL-center_pheno - Apr 2026</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI</link>
<description>BEL-center_pheno Calendar - Apr 2026</description>
<language>en</language>
<copyright>Copyright 2026, </copyright>
<item>
<uid>7mn5cu0s24jvhh38pq9ciecb8s@google.com</uid>
<event_start>12:15 PM</event_start>
<title>Wed Apr 1 2026: ULB PhysTH Seminar, Spencer Griffith [Ohio State University, USA],  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260401&amp;cal=BEL-center_pheno</link>
<description>Wed Apr 1 2026 12:15 PM: Minimal Dark Matter: Generalized Framework and Direct-Detection Sensitivity&lt;br&gt;&lt;br&gt;Numerous models of particle dark matter have been proposed, many of&lt;br&gt;which remain viable given current experimental and observational&lt;br&gt;constraints. Minimal dark matter is an extremely attractive option since&lt;br&gt;it envisions the addition of a single SU(2) multiplet to the standard&lt;br&gt;model, rather than a complicated array of particles and interactions.&lt;br&gt;However, experimental limits already rule out a subset of minimal dark&lt;br&gt;matter possibilities and are approaching the predicted phase space of&lt;br&gt;the remaining candidates. We consider extensions to the minimal dark&lt;br&gt;matter paradigm, particularly a combination of two multiplets with a&lt;br&gt;Higgs coupling, and the non-perturbative effects which may alleviate&lt;br&gt;this experimental pressure.&lt;br&gt;</description>
</item>
<item>
<uid>3rmbdqfo7ich7q9jcd8cfgiakd@google.com</uid>
<event_start>12:15 PM</event_start>
<title>Wed Apr 8 2026: ULB PhysTH Journal Club, Fabien [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260408&amp;cal=BEL-center_pheno</link>
<description>Wed Apr 8 2026 12:15 PM: </description>
</item>
<item>
<uid>48iuq2a8cgs7cf5q4h5ghu9rr9@google.com</uid>
<event_start>11:00 AM</event_start>
<title>Fri Apr 10 2026: ULB PhysTH Seminar, Pablo Sesma [IFAE, Barcelona],  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260410&amp;cal=BEL-center_pheno</link>
<description>Fri Apr 10 2026 11:00 AM: Title: Weak Scale Triggers in the SMEFT</description>
</item>
<item>
<uid>3rmbdqfo7ich7q9jcd8cfgiakd@google.com</uid>
<event_start>12:15 PM</event_start>
<title>Wed Apr 15 2026: ULB PhysTH Journal Club, Chengchao [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260415&amp;cal=BEL-center_pheno</link>
<description>Wed Apr 15 2026 12:15 PM: </description>
</item>
<item>
<uid>7kl0r7rt71gp61l6u8id4ph0ot@google.com</uid>
<event_start>11:00 AM</event_start>
<title>Thu Apr 16 2026: ULB PhysTH Seminar, Mikhail Shaposhnikov [EPFL, Lausanne],  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260416&amp;cal=BEL-center_pheno</link>
<description>Thu Apr 16 2026 11:00 AM: Unifying the Higgs Mass Hierarchy, the Cosmological Constant, and the Axion Quality Puzzles</description>
</item>
<item>
<uid>11d1f2is0074tei8iofusm4f1p@google.com</uid>
<event_start>11:00 AM</event_start>
<title>Fri Apr 17 2026: ULB PhysTH Seminar, Pratika Dayal [CITA, University of Toronto],  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260417&amp;cal=BEL-center_pheno</link>
<description>Fri Apr 17 2026 11:00 AM: &lt;b&gt;The emergence of galaxies in the first billion years&lt;/b&gt;&lt;br&gt;&lt;br&gt;Galaxy formation in the first billion years marks a time of great upheaval in our cosmic history: the first sources of light in the Universe, these galaxies ended the &#039;cosmic dark ages&#039; and produced the first photons that could break apart the hydrogen atoms suffusing all of space starting the process of &#039;cosmic reionization&#039;. The past few years have seen cutting-edge instruments such as the James Webb Space Telescope (JWST) provide tantalising glimpses of such galaxies assembling in an infant Universe. Puzzlingly, these observations are also yielding a sample of unexpectedly numerous and large black holes (up to a 100 million solar masses) within the first 600 million years, posing an enormous challenge for galaxy formation models. I will show how this data is providing an unprecedented opportunity to pin down the reionization state of the Universe in addition to providing an unrivalled resource for understanding the reioni</description>
</item>
<item>
<uid>3rmbdqfo7ich7q9jcd8cfgiakd@google.com</uid>
<event_start>12:15 PM</event_start>
<title>Wed Apr 22 2026: ULB PhysTH Journal Club,  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260422&amp;cal=BEL-center_pheno</link>
<description>Wed Apr 22 2026 12:15 PM: </description>
</item>
<item>
<uid>3rmbdqfo7ich7q9jcd8cfgiakd@google.com</uid>
<event_start>12:15 PM</event_start>
<title>Wed Apr 29 2026: ULB PhysTH Journal Club,  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20260429&amp;cal=BEL-center_pheno</link>
<description>Wed Apr 29 2026 12:15 PM: </description>
</item>
</channel>
</rss>
