Enabling Thermal Dark Matter within the Vanilla $L_μ$-$L_τ$ Model

Fuente: arXiv
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Auteurs principaux: Bernal, Nicolás, Neto, Jacinto P., Silva-Malpartida, Javier, Queiroz, Farinaldo S.
Format: Preprint
Publié: 2025
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author Bernal, Nicolás
Neto, Jacinto P.
Silva-Malpartida, Javier
Queiroz, Farinaldo S.
author_facet Bernal, Nicolás
Neto, Jacinto P.
Silva-Malpartida, Javier
Queiroz, Farinaldo S.
contents Thermal dark matter is a compelling setup that has been probed by a multitude of experiments, mostly in the GeV-TeV mass range. The thermal paradigm in the sub-GeV range is about to experience the same experimental test with the next generation of low-energy accelerators and light dark matter detectors. Motivated by this, we investigate thermal dark matter in the $L_μ-L_τ$ and assess how the introduction of a matter-dominated era impacts the parameter that yields the correct relic density. Interestingly, we show that the projected experiments, such as MuSIC, FCC-ee, and LDMX, will probe a large region of the viable parameter space that yields the correct relic density. In the GeV-TeV mass regime, the usual large-scale detectors push the sensitivity. Our work highlights the rich interplay between early-universe dynamics, dark matter phenomenology, and the discovery potential of next-generation experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2507_02048
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Enabling Thermal Dark Matter within the Vanilla $L_μ$-$L_τ$ Model
Bernal, Nicolás
Neto, Jacinto P.
Silva-Malpartida, Javier
Queiroz, Farinaldo S.
High Energy Physics - Phenomenology
Thermal dark matter is a compelling setup that has been probed by a multitude of experiments, mostly in the GeV-TeV mass range. The thermal paradigm in the sub-GeV range is about to experience the same experimental test with the next generation of low-energy accelerators and light dark matter detectors. Motivated by this, we investigate thermal dark matter in the $L_μ-L_τ$ and assess how the introduction of a matter-dominated era impacts the parameter that yields the correct relic density. Interestingly, we show that the projected experiments, such as MuSIC, FCC-ee, and LDMX, will probe a large region of the viable parameter space that yields the correct relic density. In the GeV-TeV mass regime, the usual large-scale detectors push the sensitivity. Our work highlights the rich interplay between early-universe dynamics, dark matter phenomenology, and the discovery potential of next-generation experiments.
title Enabling Thermal Dark Matter within the Vanilla $L_μ$-$L_τ$ Model
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2507.02048