Unlocking the Inelastic Dark Matter Window with Vector Mediators
Ana Luisa Foguel, Peter Reimitz, and Renata Zukanovich Funchal

TL;DR
This paper explores inelastic dark matter models with general vector mediators, revealing new viable parameter spaces and providing computational tools to analyze relic densities, thereby expanding the experimental search landscape.
Contribution
It introduces the study of inelastic dark matter with general vector mediators, including models with baryon and lepton number couplings, and offers a Python library for relic density calculations.
Findings
New viable parameter regions for inelastic dark matter models.
Anomaly-free gauge groups with non-universal lepton couplings open unexplored parameter space.
Provision of a Python library for relic density computation.
Abstract
Despite the robust cosmological and astrophysical evidence confirming the existence of a non-baryonic matter component in the Universe, the underlying nature of Dark Matter (DM) remains a mystery. Among the several possible scenarios, light DM candidates thermally produced in the early Universe are especially interesting, since their abundance could be set via the standard freeze-out mechanism. Additionally, new light states can present a rich phenomenology and are attracting increasing attention due to recent experimental capabilities to probe dark sectors with feeble interactions. In particular, inelastic DM (iDM) candidates are an appealing option, since they can avoid cosmic microwave background (CMB) radiation bounds as well as indirect and direct detection searches. Although such models have been intensively studied in the literature, the usual scenario is to consider a secluded…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Scientific Research and Discoveries · Cosmology and Gravitation Theories
