Asymmetric dark matter from leptogenesis in type-III seesaw framework with modular $S_4$ symmetry
Abhishek, V. Suryanarayana Mummidi

TL;DR
This paper proposes a unified model linking neutrino masses, baryogenesis, and dark matter using modular $S_4$ symmetry and type-III seesaw, predicting observable neutrino parameters and explaining cosmic matter asymmetry.
Contribution
It introduces a novel framework where a single complex modulus controls flavor, CP violation, and matter-antimatter asymmetry, providing testable predictions for neutrino and dark matter properties.
Findings
Reproduces neutrino oscillation data within 3σ NuFIT ranges.
Predicts baryon asymmetry and dark matter relic density consistent with observations.
Suggests dark matter mass around 0.1-2 GeV, testable in future experiments.
Abstract
We present a unified framework for neutrino masses, baryogenesis, and dark matter based on a modular symmetry combined with a type-III seesaw mechanism. All Yukawa couplings, CP phases, and flavor textures originate from a single complex modulus , whose vacuum expectation value controls both visible and dark sector dynamics. The same modular parameter fixes the neutrino mass matrix, determines the CP asymmetries driving resonant leptogenesis, and correlates the resulting baryon and dark matter abundances. A detailed numerical analysis shows that the model reproduces all neutrino oscillation data within the NuFIT~5.2 (2024) ranges for normal ordering, predicting , , and an effective Majorana mass , testable in…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Neutrino Physics Research
