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Dark Matter Physics from the CMB-S4 Experiment
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The nature of dark matter is one of the major puzzles of fundamental physics, integral to the understanding of our universe across almost every epoch. The search for dark matter takes place at different energy scales, and use data ranging from particle colliders to astrophysical surveys. We focus here on CMB-S4, a future ground-based Cosmic Microwave Background (CMB) experiment, which is expected to provide exquisite measurements of the CMB temperature and polarization anisotropies. These measurements (on their own and in combination with other surveys) will allow for new means to shed light on the nature of dark matter.
Forward citations
Cited by 2 Pith papers
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Probing the Phenomenology of Dark Matter from Decoupled Freeze-Out
In a scalar-plus-pseudoscalar mediator model, decoupled freeze-out can produce the observed dark matter relic density via s-wave annihilation while evading CMB limits, though indirect-detection and BBN bounds leave on...
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J-PLUS: Tomographic analysis of galaxy angular density and redshift fluctuations in Data Release 3. Constraints on photo-$z$ errors, linear bias, and peculiar velocities
Tomographic fits to J-PLUS DR3 angular density and redshift fluctuations give galaxy bias rising from 0.9 to 1.5 between z=0.05 and z=0.15 and photo-z errors about 40% larger than LePhare's estimate.
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