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<title>BEL-center_pheno - Week of 11/08/2026</title>
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<description>BEL-center_pheno Calendar - Week of 11/08/2026</description>
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<title>Fri Nov 13 2026: ULB PhysTH Seminar, Arpan Kar [ULB],  [BEL-center:pheno]</title>
<link>http://cp3.irmp.ucl.ac.be:80/PAI/day.php?getdate=20261113&amp;cal=BEL-center_pheno</link>
<description>Fri Nov 13 2026 11:00 AM: &lt;b&gt;Unveiling Dark Matter Interactions through MeV Gamma-Ray Astronomy&lt;/b&gt;&lt;br&gt;&lt;br&gt;Dark Matter (DM) particles (with MeV - TeV masses) annihilating in the Galactic halo not only produce gamma-rays via prompt radiation, but also generate abundant e+-&#039;s, which subsequently emit through inverse Compton scattering, bremsstrahlung and in-flight annihilation processes, collectively called `secondary emissions&#039;. While the prompt gamma-rays concentrate at a higher energy, the secondary emissions give rise to a broad photon spectrum ranging from hard X-rays to gamma-rays, which the upcoming space-based MeV telescopes will be able to probe. I shall discuss the sensitivity of these telescopes for &#039;weak-scale&#039; DM particles with GeV - TeV masses, as well as for &#039;sub-GeV&#039; DM with MeV - GeV masses (based on realistic models). I shall show that the MeV telescopes are able to probe a wide region of the DM parameter space which is currently unconstrained by other observations. I shall also discuss the compleme</description>
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