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Speaker Tipo de Evento
Mayo 16 2024 - 15:00 Probing new physics with Galactic (keV-MeV) gamma-ray emission Pedro de la Torre Luque Measurements of the 511 keV emission reveal the presence of a steady injection of positrons that is very concentrated around the Galactic bulge, and whose origin remains unknown. Seminar
Mayo 20 2024 - 15:00 Extracting Scattering Amplitudes from Euclidean Correlators Agostino Patella Scattering amplitudes can be extracted from time-ordered n-point functions by means of the well known LSZ reduction formula, even in non-perturbative Quantum Field Theories, such as Quantum Chromod Seminar
Mayo 21 2024 - 11:30 Dark Matter in the Universe Katherine Freese The nature of the dark matter in the Universe is among the longest and most important outstanding problems in all of modern physics. Colloquium
Mayo 21 2024 - 14:00 Cosmology/gravity journal club Join the IFT cosmology/gravity journal club at https://benty-fields.com to vote for papers and volunteer to present them. CosmoGrav Journal Club
Mayo 22 2024 - 11:30 A brief introduction to symmetry-protected topological phases Hua-Chen Zhang (IFT) "I will give a brief introductory presentation on the topic of symmetry-protected topological (SPT) phases [mainly in (1+1)D], with an emphasis on the relevant concepts, including the definition of Quantum Information Journal Club
Mayo 23 2024 - 12:00 SPLE Club Paper discussion. SPLE-Club
Mayo 23 2024 - 15:00 Sub-GeV dark matter and relic neutrinos at high energies Filippo Sala Dark matter (DM) below a GeV is motivated by some cosmological histories and possibly by anomalies in data. Leading detectors cannot easily test it, due to its small kinetic energy. Seminar
Mayo 27 2024 - 15:00 TBA James M. Cline Seminar
Mayo 28 2024 - 14:00 Cosmology/gravity journal club
CosmoGrav Journal Club
Mayo 30 2024 - 15:00 HNLs from Heavy ALP decays at Neutrino Facilities Asli Abdullahi We present a chiral non-abelian dark sector model that features a spontaneous $SU(3)\times SU(2) \rightarrow SU(3)$ symmetry breaking and results in the formation of dark mesons, $\pi_D$, and baryo Seminar

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