LZ Paper Map248 keV papers & summaries

Comparisons & systematics · Discriminant

LMC-Perturbed LZ Dark Matter Landscape

Nassim Bozorgnia, Samantha Contreras, Graciela B. Gelmini, Alvine C. Kamaha, Javier Reynoso-Cordova, Yongheng Xu

Published
September 28, 2026
Identifier
arXiv:2609.36184

Why it is here

LMC-induced halo structure changes which inelastic splittings remain viable and strengthens the case for model-specific astrophysical treatment.

Machine-assisted summary

The authors propagate a Large-Magellanic-Cloud-enhanced high-speed tail through a range of event interpretations, finding sizeable shifts for endothermic models while elastic candidates are comparatively stable.

Large Magellanic Cloudhigh-velocity tailendothermic dark matterhalo uncertainty

Citation lineage on this map

Cites 32

Cited by 2

Metadata comes from arXiv. Summaries and placement are machine-assisted; inclusion is not endorsement or peer review.