Although the Standard Model (SM) has been remarkably successful, several theoretical and phenomenological challenges remain unresolved. A major issue is the absence of a viable dark matter (DM) candidate, despite strong indirect evidence for its existence from galactic and cluster-scale observations. Another open question is the observed matter–antimatter asymmetry: while the SM can generate such an asymmetry, the predicted amount falls short of observations. Asymmetric dark matter provides a compelling framework to address both problems simultaneously, particularly given that observations indicate the DM abundance is only about five times larger than that of ordinary matter. In this work, we propose a supersymmetric model that naturally accommodates this mechanism.
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