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Dr Joshua Green (University College London)19/10/2026 14:20Dark Universe
The LUX-ZEPLIN experiment is a liquid-gas dual phase time projection chamber primarily searching for dark matter in the form of weakly interacting massive particles (WIMPs). It has been collecting science data with a 7-tonne active xenon target near-continuously since 2021. LZ has reported world-leading WIMP dark matter searches, a measurement of coherent solar $^8$B neutrino scattering on...
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MATTIA DI MAURO (INFN TORINO)19/10/2026 14:55Dark Universe
The recent high-energy recoil event reported by LUX-ZEPLIN has motivated a broad range of dark-matter interpretations. In this talk I will review the main theoretical scenarios that have been proposed, including thermal Higgsino and minimal electroweak dark matter, pseudo-Dirac models, endothermic and exothermic dark matter, and elastic momentum-dependent interactions.
I will focus in...
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cervane grimaud (IRFU / CEA Paris-Saclay)19/10/2026 16:05Dark Universe
Axion-Like Particles (ALPs) are well-motivated candidates for light dark matter and may couple with photons in the presence of astrophysical magnetic fields which give rise to the possibility of photon-ALP oscillations. If sufficiently strong, this mixing can induce characteristic energy-dependent feature in gamma-ray spectrum of astrophysical sources.
In this work, we explore the...
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Ana Foguel (University of Bologna)19/10/2026 16:30Dark Universe
The Standard Model (SM) of particle physics remains an incomplete theory, with the nature of dark matter (DM) among its major open questions. Guided by symmetry and simplicity, a new dark sector can communicate with the SM through three renormalizable portals: vector, scalar and neutrino. In particular, the vector portal is among the minimal realizations, with the standard dark photon as its...
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Thomas REGGIO (LPCA)19/10/2026 16:55Dark Universe
The Inert Doublet Model (IDM) is one of the most studied models of frozen-out WIMP dark matter. In this talk we will see that, depending on the thermal history of the universe, the IDM dark matter candidate can effectively behave as a FIMP despite being charged under the electroweak gauge group. We will discuss the DM abundance predicted by the IDM under different cosmological assumptions and...
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