Project B3a will explore the phenomenology of dark sector models that address the dark matter problem by introducing new particles with very weak couplings to the Standard Model but potentially strong interactions between them. We will calculate predictions for collider signatures, such as dark showers or displaced vertices, and for observables at flavour experiments, such as rare decays. These predictions will then be compared to experimental data and combined with cosmological and astrophysical observations in order to perform global fits of dark sector models.
Topics
Models: light WIMPs
Motivation and constraints for GeV-scale dark matter
Embedding of simplified models into full theories
Models: Beyond WIMPs
Exploration of the different dark matter production mechanisms
Connection between the structure of dark sectors to exotic signatures
Phenomenology: Resonance searches
Identification of the most sensitive observables and signal regions
Inclusion of searches for broad resonances and displaced vertices
Phenomenology: (Dark) showers
Simulation of light dark matter annihilation with HERWIG
Development of a tool to simulate dark showers based on HERWIG
Interpretation: Recasting
Combination of all relevant LHC searches and flavour observables
Constraints on dark sectors from SM precision measurements
Interpretation: Global fits
Viability of WIMP models and predictions for future WIMP searches
Framework to analyse complementary information and positive signals dictions and advanced searches.
Related publications
P3H-22-033
Title: Forecasting dark showers at Belle II
Type: Paper
Authors: Elias Bernreuther, Kai Böse, Torben Ferber, Christopher Hearty, Felix Kahlhoefer, Alessandro Morandini, Kai Schmidt-Hoberg
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