activity
20242026
collaborators

6 papers

hep-ph2026

Directional dark matter signatures of the Large Magellanic Cloud

Javier Reynoso-Cordova, Nassim Bozorgnia, Marie-Cécile Piro

The Large Magellanic Cloud (LMC), the most massive satellite of the Milky Way (MW), can significantly perturb the local dark matter (DM) distribution. We study its impact on direct…

hep-ex2026

Demonstration of Efficient Radon Removal by Silver-Zeolite in a Dark Matter Detector

Daniel Durnford, Yuqi Deng, Carter Garrah +6

We present the performance of an efficient radon trap using silver-zeolite Ag-ETS-10, measured with a spherical proportional counter filled with an argon/methane mixture. Our study…

physics.ins-det2025

Calibration Plan for the SBC 10-kg Liquid Argon Detector with 100 eV Target Threshold

E. Alfonso-Pita, D. Baxter, E. Behnke +32

The Scintillating Bubble Chamber (SBC) Collaboration is designing a new generation of low background, noble liquid bubble chamber experiments with sub-keV nuclear recoil threshold.…

hep-ph2024

Cosmic Ray Muons in Laboratories Deep Underground

William Woodley, Anatoli Fedynitch, Marie-Cécile Piro

We provide comprehensive calculations of total muon fluxes, energy and angular spectra, and mean muon energies in deep underground laboratories - under flat overburdens and mountai…

hep-ph2024

The Large Magellanic Cloud: expanding the low-mass parameter space of dark matter direct detection

Javier Reynoso-Cordova, Nassim Bozorgnia, Marie-Cécile Piro

We investigate how the Large Magellanic Cloud (LMC) impacts the predicted signals in near-future direct detection experiments for non-standard dark matter (DM) interactions, using…

hep-ph2024

Model for bubble nucleation efficiency of low-energy nuclear recoils in bubble chambers for dark matter detection

Xiang Li, Marie-Cécile Piro

Bubble chambers are promising technologies for detecting low-energy nuclear recoils from the elastic scattering of dark matter particle candidates. Bubble nucleation occurs when th…