Hunting for heavy $Z^\prime$ with IceCube neutrinos and gravitational waves
Basabendu Barman, Arindam Das, Suruj Jyoti Das, and Marco Merchand

TL;DR
This paper proposes a unified model where PeV-scale dark matter decay explains IceCube neutrino events, baryon asymmetry is generated via leptogenesis, and gravitational waves from cosmic strings provide testable signals, linking particle physics and cosmology.
Contribution
It introduces a minimal gauged B-L extension that simultaneously explains dark matter decay, baryon asymmetry, and predicts gravitational wave signals from cosmic strings.
Findings
Dark matter decay accounts for IceCube neutrino observations.
Leptogenesis from right-handed neutrinos explains baryon asymmetry.
Gravitational wave spectrum links symmetry-breaking scale to observable signals.
Abstract
In the minimal gauged B-L extension of the Standard Model, we demonstrate that PeV-scale dark matter (DM) and the baryon asymmetry of the Universe (BAU) can be simultaneously explained through the three right-handed neutrinos (RHNs) present in the theory. The DM candidate undergoes decay into light neutrinos, providing an explanation for the observed IceCube events, while the other two RHNs generate the BAU via leptogenesis. The breaking of gauge symmetry gives rise to detectable gravitational waves (GWs) from decaying cosmic strings (CS), making this framework testable at several future GW detectors-despite being beyond the reach of conventional collider experiments due to the extremely weak coupling. The symmetry-breaking scale establishes a connection between particle masses, couplings, and the GW spectrum, offering a unified and predictive scenario.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Computational Physics and Python Applications · Particle physics theoretical and experimental studies
